Solar eclipse of August 11, 1999

Solar eclipse of August 11, 1999
Solar eclipse of August 11, 1999
	Totality from France
	Map
Type of eclipse
Nature	Total
Gamma	0.5062
Magnitude	1.0286
Maximum eclipse
Duration	143 s (2 min 23 s)
Location	Ocnele Mari, Vâlcea County, Romania
Coordinates	45°06′N24°18′E / 45.1°N 24.3°E
Max. width of band	112 km (70 mi)
Times (UTC)
Greatest eclipse	11:04:09
References
Saros	145 (21 of 77)
Catalog # (SE5000)	9506

Last updated April 11, 2024

A total solar eclipse occurred on 11 August 1999 with an eclipse magnitude of 1.0286. A solar eclipse occurs when the moon passes between earth and the sun, thereby totally or partly obscuring the image of the sun for a viewer on earth. A total solar eclipse occurs when the moon's apparent diameter is larger than the sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. The path of the moon's shadow began in the Atlantic Ocean and, before noon, was traversing the southern United Kingdom, northern France, Belgium, Luxembourg, southern Germany, Austria, Slovenia, Croatia, Hungary, and northern FR Yugoslavia (Vojvodina). The eclipse's maximum was at 11:03 UTC at 45°06′N24°18′E / 45.1°N 24.3°E / 45.1; 24.3 in Romania (next to the town of Ocnele Mari near Râmnicu Vâlcea);^[1]^[2]^[3] and it continued across Bulgaria, the Black Sea, Turkey, the northeastern tip of Syria, northern Iraq, Iran, southern Pakistan and Srikakulam in India and ended in the Bay of Bengal.

Observations

The eclipse as seen from France

Interactive map of the path of the Umbral Shadow

Because of the high population densities in areas of the path, this was one of the most-viewed total solar eclipses in human history;^[4] although some areas in the path of totality (mainly in Western Europe) offered impaired visibility due to adverse weather conditions.

Some of the organized eclipse-watching parties along the path of totality set up video projectors on which people could watch the moon's shadow as it raced towards them.^[5] There was substantial coverage on international TV stations of the progress of the eclipse shadow. The moon's shadow was also observed from the Russian Mir space station; during the eclipse, video from Mir was broadcast live on television.

The BBC concentrated its coverage efforts on the first landfall of the shadow across the western end of Cornwall (from St Ives to Lizard), which was packed with an extraordinary number of visitors, although Cornwall did not have nearly as many spectators as expected leading many organised events to host smaller audiences than anticipated. The veteran amateur astronomer, broadcaster and eclipse-watcher Patrick Moore was brought in to head a live programme, but the eclipse was clouded out. BBC One also produced a special version of their Balloon Idents for the event. The BBC did not have a presence at Goonhilly on the Lizard Peninsula, one of the few places in Cornwall where the clouds parted just in time for the total eclipse to be visible. There was extensive cloud in Perranporth which parted just in time, allowing the very large crowd that had filled the beach and hillsides to witness the event.
Some of the best viewing conditions were to be had mid-Channel, where ferries were halted in calm conditions to obtain an excellent view. Hundreds of people who gathered on the island of Alderney also experienced the event.
Also at sea, many of the Fastnet fleet contestants encountered totality crossing the Celtic Sea on their way to the Fastnet Rock.^[6]
A gathering of several thousand people at the airport in Soissons, France, which was on the path of totality, were denied all but a few fleeting glimpses of the eclipse through the overcast sky. The clouds cleared completely just a few minutes after the eclipse.
In contrast, the overcast sky in Amiens, France, where thousands had gathered, cleared only minutes before the eclipse began.
Further inland, viewing conditions were also perfect at Vouziers, a French country town gridlocked by Belgian cars from day-visitors. The patchy cloud covering cleared a short time before the shadow arrived. Some photos from Vouziers were used on the subsequent BBC Sky at Night programme.
The San Francisco Exploratorium featured a live webcast from a crowded town square in Amasya, Turkey.
Doordarshan, the national TV channel in India, broadcast live coverage from Srikakulam, hosted by TV personality Mona Bhattacharya.
A Bulgarian Air Force MiG-21 two-seater was used by the Bulgarian Academy of Sciences to study the solar corona. The MiG-21, flying at 1600–1700 km/h (1000 to 1100 mph) (M=1,4-1,5) at an altitude of 13,000 metres (43,000'), was able to stay in the moon's umbra for 6 min. The photographer, an air force pilot, used two film cameras, both fitted with 200 mm lenses and infrared filters, and one Digital8 video camera.
Hungary's most popular tourist destination, Lake Balaton and its surrounding area, fell into the path of the eclipse entirely, which made the area even more popular for the day. The motorway leading to the city was so crowded that many people had to watch the eclipse while caught in a traffic jam.
One French and two British Concordes briefly followed the eclipse with tourists on board.^[7]
The BBC was filming one of its episodes for the TV series Airport that day and, during the show, resident press officers Russell Clisby and Steve Meller took photographs of the eclipse at Heathrow Airport, as well as Aeroflot supervisor Jeremy Spake witnessing the eclipse on a special charter flight.
RTS, the national public broadcaster of Serbia, urged people to remain inside, citing dangers to public health. This caused the streets of all Serbian cities, towns and villages to be entirely deserted during the eclipse, with many opting to watch it on TV instead.^[8]
The BMJ, a month after the eclipse, reported only 14 cases of eye damage from improper viewing of the eclipse - a number lower than initially feared. In one of the most serious cases the patient had looked at the sun without eye protection for twenty minutes, but overall the public health campaign had succeeded.^[9]

Gallery

Salzburg, Austria
Partial from Paderborn, Germany
Partial from Oria, Italy
Partial from Haarlem, the Netherlands
Projection in Oslo, Norway
Lake Balaton, Hungary
Laon, France

Notable times and coordinates

Animated path SE1999Aug11T.gif — Animated path

Event	Time (UTC)	Coordinates^[10]
1st penumbral contact with Earth's surface (P1)	08:26:17
1st external umbral contact (U1)	09:29:55	41°2.0′N65°5.4′W / 41.0333°N 65.0900°W / 41.0333; -65.0900
2nd internal umbral contact (U2)	09:30:53	43°0.1′N57°55.8′W / 43.0017°N 57.9300°W / 43.0017; -57.9300
Greatest eclipse	11:03:07	45°4.8′N24°17.3′E / 45.0800°N 24.2883°E / 45.0800; 24.2883 ^[11]
3rd internal umbral contact (U3)	12:35:33	19°39.7′N80°20.4′E / 19.6617°N 80.3400°E / 19.6617; 80.3400
4th external umbral contact (U4)	12:36:26	17°33.5′N87°17.1′E / 17.5583°N 87.2850°E / 17.5583; 87.2850
4th penumbral contact with Earth's surface (P4)	13:40:08

Related eclipses

Eclipses of 1999

A penumbral lunar eclipse on January 31.
An annular solar eclipse on February 16.
A partial lunar eclipse on July 28.
A total solar eclipse on August 11.

Solar eclipses 1997–2000

This eclipse is a member of a semester series. An eclipse in a semester series of solar eclipses repeats approximately every 177 days and 4 hours (a semester) at alternating nodes of the Moon's orbit.^[12]

Solar eclipse series sets from 1997 to 2000
Saros	Map	Gamma	Saros	Map	Gamma
Descending node			Ascending node
120 Chita, Russia	1997 March 09 Total	0.91830	125	1997 September 02 Partial (south)	−1.03521
130 Total eclipse near Guadeloupe	1998 February 26 Total	0.23909	135	1998 August 22 Annular	−0.26441
140	1999 February 16 Annular	−0.47260	145 Totality from France	1999 August 11 Total	0.50623
150	2000 February 05 Partial (south)	−1.22325	155	2000 July 31 Partial (north)	1.21664

Partial solar eclipses on July 1, 2000 and December 25, 2000 occur in the next lunar year eclipse set.

Saros 145

This solar eclipse is a part of Saros cycle 145, repeating every 18 years, 11 days, 8 hours, containing 77 events. The series started with a partial solar eclipse on January 4, 1639, and reached a first annular eclipse on June 6, 1891. It was a hybrid event on June 17, 1909, and total eclipses from June 29, 1927, through September 9, 2648. The series ends at member 77 as a partial eclipse on April 17, 3009. The longest eclipse will occur on June 25, 2522, with a maximum duration of totality of 7 minutes, 12 seconds. All eclipses in this series occurs at the Moon's ascending node.

Series members 10–32 occur between 1801 and 2359
10	11	12
April 13, 1801	April 24, 1819	May 4, 1837
13	14	15
May 16, 1855	May 26, 1873	June 6, 1891
16	17	18
June 17, 1909	June 29, 1927	July 9, 1945
19	20	21
July 20, 1963	July 31, 1981	August 11, 1999
22	23	24
August 21, 2017	September 2, 2035	September 12, 2053
25	26	27
September 23, 2071	October 4, 2089	October 16, 2107
28	29	30
October 26, 2125	November 7, 2143	November 17, 2161
31	32	33
November 28, 2179	December 9, 2197	December 21, 2215
34	35	36
December 31, 2233	January 12, 2252	January 22, 2270
37	38	39
February 2, 2288	February 14, 2306	February 25, 2324
40
March 8, 2342

Metonic series

The metonic series repeats eclipses every 19 years (6939.69 days), lasting about 5 cycles. Eclipses occur in nearly the same calendar date. In addition, the octon subseries repeats 1/5 of that or every 3.8 years (1387.94 days). All eclipses in this table occur at the Moon's ascending node.

22 eclipse events between January 5, 1935 and August 11, 2018
January 4-5	October 23-24	August 10-12	May 30-31	March 18-19
111	113	115	117	119
January 5, 1935		August 12, 1942	May 30, 1946	March 18, 1950
121	123	125	127	129
January 5, 1954	October 23, 1957	August 11, 1961	May 30, 1965	March 18, 1969
131	133	135	137	139
January 4, 1973	October 23, 1976	August 10, 1980	May 30, 1984	March 18, 1988
141	143	145	147	149
January 4, 1992	October 24, 1995	August 11, 1999	May 31, 2003	March 19, 2007
151	153	155
January 4, 2011	October 23, 2014	August 11, 2018

Popular culture

Sleeping Sun (1999), by the Finnish band Nightwish
Les Terriens (2000), French documentary directed by Ariane Doublet
Les Ensoleillés (2002), compilation of around twenty short stories based on the 1999 eclipse, written by Joël Egloff

Notes

↑ Stavinschi, M., National Seminar" The total solar Eclipse of August, 11, 1999. Interdisciplinary approach, Bucharest, October 15, 1998 in: Romanian Astron. J., vol.8, N.2, p.146 (1998)
↑ Scientific session " Eclipsa 99", Romanian Astronomical Journal, vol.9, N.1, p.103 (1999)
↑ Stavinschi, M., The maximum of the last eclipse of the Millenium was in Romania, Romanian Astronomical Journal, , vol.9, N.2, p.109- 114, 1999
↑ "Solar show in sky or on the Internet". 10 August 1999.
↑ "ISMB 99". Bioinf.mpi-sb.mpg.de. Retrieved 2013-10-01.
↑ "Boats warned of freak winds during eclipse". Guardian. 7 June 1999. Archived from the original on 17 October 2015.
↑ Hatherill, Chris (9 March 2016). "When Astronomers Chased a Total Eclipse in a Concorde". Vice . Retrieved 10 March 2016.
↑ Janković, Vladimir (July 2010). "Atmosfear: Slobodan Milošević versus 1999 Solar Eclipse". Centre for the History of Science, Technology of Medicine.
↑ Dobson, Roger (1999-08-21). "UK hospitals assess eye damage after solar eclipse". The BMJ. 319 (7208): 469. doi:10.1136/bmj.319.7208.469. PMC 1116382 . PMID 10454393.
↑ "Eclipse2017 - Total Solar Eclipse 2017". eclipse.gsfc.nasa.gov.
↑ "Eclipse2017 - Total Solar Eclipse 2017". eclipse.gsfc.nasa.gov.
↑ van Gent, R.H. "Solar- and Lunar-Eclipse Predictions from Antiquity to the Present". A Catalogue of Eclipse Cycles. Utrecht University. Retrieved 6 October 2018.

Related Research Articles

<span class="mw-page-title-main">Solar eclipse of March 29, 2006</span> 21st-century total solar eclipse

A total solar eclipse occurred on March 29, 2006. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. It was visible from a narrow corridor which traversed half the Earth. The magnitude, that is, the ratio between the apparent sizes of the Moon and that of the Sun, was 1.052, and it was part of Saros 139.

A total solar eclipse took place on Sunday, November 23, 2003, with a magnitude of 1.0379. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. It was visible from a corridor in the Antarctic region. A partial eclipse was seen from the much broader path of the Moon's penumbra, including the southern tip of South America and most of Australia.

<span class="mw-page-title-main">Solar eclipse of December 4, 2002</span> 21st-century total solar eclipse

A total solar eclipse took place on December 4, 2002, with a magnitude of 1.0244. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. It was visible from a narrow corridor in southern Africa, the Indian Ocean and southern Australia. A partial eclipse was seen from the much broader path of the Moon's penumbra, including most of Africa and Australia. During the sunset after the eclipse many observers in Australia saw numerous and unusual forms of a green flash.

A total solar eclipse took place on June 21, 2001, with a magnitude of 1.0495. It was the first solar eclipse of the 21st century. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. Occurring 2.2 days before perigee, the Moon's apparent diameter was larger.

<span class="mw-page-title-main">Solar eclipse of October 3, 2005</span> 21st-century annular solar eclipse

An annular solar eclipse occurred at the Moon's descending node of the orbit on October 3, 2005, with a magnitude of 0.958. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide. Occurring only 4.8 days after apogee, the Moon's apparent diameter was smaller. It was visible from a narrow corridor through the Iberian peninsula and Africa and Brazil. A partial eclipse was seen from the much broader path of the Moon's penumbra, including all of Europe, Africa and southwestern Asia. The Sun was 96% covered in a moderate annular eclipse, lasting 4 minutes and 32 seconds and covering a broad path up to 162 km wide. The next solar eclipse in Africa occurred just 6 months later.

<span class="mw-page-title-main">Solar eclipse of April 8, 2005</span> 21st-century total solar eclipse

A total solar eclipse occurred at the Moon's ascending node on April 8, 2005. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. This eclipse is a hybrid event, a narrow total eclipse, and beginning and ending as an annular eclipse.

The total solar eclipse of July 11, 2010 occurred over the southern Pacific Ocean. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide.

<span class="mw-page-title-main">Solar eclipse of August 1, 2008</span> 21st-century total solar eclipse

A total solar eclipse occurred at the Moon's descending node of the orbit on August 1, 2008. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. It had a magnitude of 1.0394 that was visible from a narrow corridor through northern Canada (Nunavut), Greenland, central Russia, eastern Kazakhstan, western Mongolia and China. Visible north of the Arctic Circle, it belonged to the so-called midnight sun eclipses. The largest city in its path was Novosibirsk in Russia. The eclipse happened only 2+1⁄2 days after the perigee that occurred on July 29, 2008, and the Moon's apparent diameter was larger than average.

<span class="mw-page-title-main">Solar eclipse of July 11, 1991</span> 20th-century total solar eclipse

A total solar eclipse occurred at the Moon’s descending node of the orbit on Thursday, July 11, 1991. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. Totality began over the Pacific Ocean and Hawaii moving across Mexico, down through Central America and across South America ending over Brazil. It lasted for 6 minutes and 53.08 seconds at the point of maximum eclipse. There will not be a longer total eclipse until June 13, 2132. This was the largest total solar eclipse of Solar Saros series 136, because eclipse magnitude was 1.07997.

A total solar eclipse occurred on March 20, 2015. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with a partial solar eclipse visible over a surrounding region thousands of kilometres wide. This total solar eclipse is notable in that the path of totality passed over the North Pole. Totality was visible in the Faroe Islands and Svalbard.

An annular solar eclipse occurred on Tuesday, April 29, 2014. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide. The center of the Moon's shadow missed the Earth's South Pole, but the partial eclipse was visible from parts of Antarctica and Australia, and an annular eclipse was visible from a small part of Antarctica.

A total solar eclipse took place at the Moon's descending node of the orbit on March 8–9, 2016. If viewed from east of the International Date Line, the eclipse took place on March 8 (Tuesday) and elsewhere on March 9 (Wednesday). A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's and the apparent path of the Sun and Moon intersect, blocking all direct sunlight and turning daylight into darkness; the Sun appears to be black with a halo around it. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. The eclipse of March 8–9, 2016 had a magnitude of 1.0450 visible across an area of Pacific Ocean, which started in the Indian Ocean, and ended in the northern Pacific Ocean.

<span class="mw-page-title-main">Solar eclipse of November 3, 2013</span> 21st-century total solar eclipse

A total solar eclipse occurred at the Moon's ascending node on 3 November 2013. It was a hybrid eclipse of the Sun with a magnitude of 1.0159, with a small portion over the western Atlantic Ocean at sunrise as an annular eclipse, and the rest of the path as a narrow total solar eclipse. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A hybrid solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's in sunrise and sunset, but at Greatest Eclipse the Moon's apparent diameter is larger than the Sun's.

A total solar eclipse occurred at the Moon’s descending node of the orbit on Thursday, February 26, 1998. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. Totality was visible in the Galápagos Islands, Panama, Colombia, the Paraguaná Peninsula in northwestern Venezuela, all of Aruba, most of Curaçao and the northwestern tip of Bonaire, all of Montserrat, Guadeloupe and Antigua and Barbuda.

<span class="mw-page-title-main">Solar eclipse of July 22, 1990</span> 20th-century total solar eclipse

A total solar eclipse occurred on Sunday, July 22, 1990. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. Totality was visible in southern Finland, the Soviet Union, and eastern Andreanof Islands and Amukta of Alaska.

<span class="mw-page-title-main">Solar eclipse of August 12, 2026</span> Total solar eclipse August 12, 2026

A total solar eclipse will occur at the Moon's descending node of the orbit on Wednesday, August 12, 2026, two days past perigee, in parts of North America and almost all of Europe. The total eclipse will pass over the Arctic, Greenland, Iceland, Atlantic Ocean and northern Spain. The points of greatest duration and greatest eclipse will be just 45 km (28 mi) off the western coast of Iceland by 65°10.3' N and 25°12.3' W, where the totality will last 2m 18.21s. It will be the first total eclipse visible in Iceland since June 30, 1954, also Solar Saros series 126, and the only one to occur in the 21st century as the next one visible over Iceland will be in 2196. As lunar perigee will occur on August 10, 2026, two days before the total solar eclipse, the Moon's apparent diameter will be larger.

<span class="mw-page-title-main">Solar eclipse of September 3, 2081</span> Solar eclipse

A total solar eclipse will occur on Wednesday, September 3, 2081. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. The path of totality will begin at the Atlantic Ocean, off European mainland at 07:26:49 UTC and will end at Indonesian island of Java at 10:43:03 UTC.

A total solar eclipse occurred on October 24, 1995. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. The path of totality went through Iran, Afghanistan, Pakistan, India, southwestern tip of Bangladesh, Burma, Thailand, Cambodia, Vietnam, Spratly Islands, northeastern tip of Sabah of Malaysia, Philippines and Indonesia.

<span class="mw-page-title-main">Solar eclipse of June 11, 1983</span> 20th-century total solar eclipse

A total solar eclipse occurred at the Moon's ascending node of the orbit on June 11, 1983. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. Occurring only 48 hours before perigee, the Moon's apparent diameter was larger.

References

Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
- Google interactive map
- Besselian elements

Eclipse at hermit.org
"Club Krile Magazine", Vol. 11, 1999, "Air Group 2000" Publishing, Sofia, Bulgaria
The Total Solar Eclipse of 1999 August 11
Russia expedition

Photos

Turkey. Prof. Druckmüller's eclipse photography site
Hungary. Prof. Druckmüller's eclipse photography site
France. Prof. Druckmüller's eclipse photography site
Bulgaria
Solar Corona Shape
Exploratorium Webcast: Solar Eclipse August 11, 1999
KryssTal - Eclipse in Cornwall (UK)—totality not seen but scene photographed
Solar eclipse of August 11, 1999 Romania, shown in Romanian Maximum Card Archived August 21, 2019, at the Wayback Machine
Solar eclipse of August 11, 1999 Romania, shown in Romanian Maximum Card Archived August 21, 2019, at the Wayback Machine
Images from Turkey by Crayford Manor House Astronomical Society Archived 2013-02-09 at archive.today
A Crescent Sunrise, APOD 8/17/1999, partial eclipse from Quebec, Canada
Sun Block, APOD 8/18/1999, totality from Hungary
Light From The Dark Sun, APOD 8/19/1999, totality from Siofok, Hungary
At The Sun's Edge, APOD 8/20/1999, totality near Bagdere, Turkey
The Big Corona, APOD 4/8/2001, totality by Fred Espenak
Total Eclipse of the Active Sun, APOD 6/20/2001, from Kecel, Hungary
Diamond Ring in the Sun, APOD 6/21/2001, totality from eastern Turkey
Looking Back at an Eclipsed Earth, APOD 9/26/2004, total eclipse shadow seen from Mir spacestation, chosen as APOD again on 6/10/2007
Russian scientist observed eclipse

This page is based on this Wikipedia article
Text is available under the CC BY-SA 4.0 license; additional terms may apply.
Images, videos and audio are available under their respective licenses.

[1] Stavinschi, M., National Seminar" The total solar Eclipse of August, 11, 1999. Interdisciplinary approach, Bucharest, October 15, 1998 in: Romanian Astron. J., vol.8, N.2, p.146 (1998)

[2] Scientific session " Eclipsa 99", Romanian Astronomical Journal, vol.9, N.1, p.103 (1999)

[3] Stavinschi, M., The maximum of the last eclipse of the Millenium was in Romania, Romanian Astronomical Journal, , vol.9, N.2, p.109- 114, 1999

[4] "Solar show in sky or on the Internet". 10 August 1999.

[5] "ISMB 99". Bioinf.mpi-sb.mpg.de. Retrieved 2013-10-01.

[6] "Boats warned of freak winds during eclipse". Guardian. 7 June 1999. Archived from the original on 17 October 2015.

[7] Hatherill, Chris (9 March 2016). "When Astronomers Chased a Total Eclipse in a Concorde". Vice . Retrieved 10 March 2016.

[8] Janković, Vladimir (July 2010). "Atmosfear: Slobodan Milošević versus 1999 Solar Eclipse". Centre for the History of Science, Technology of Medicine.

[UK_Public_Health_Assessment-9] Dobson, Roger (1999-08-21). "UK hospitals assess eye damage after solar eclipse". The BMJ. 319 (7208): 469. doi:10.1136/bmj.319.7208.469. PMC 1116382 . PMID 10454393.

[10] "Eclipse2017 - Total Solar Eclipse 2017". eclipse.gsfc.nasa.gov.

[11] "Eclipse2017 - Total Solar Eclipse 2017". eclipse.gsfc.nasa.gov.

[12] van Gent, R.H. "Solar- and Lunar-Eclipse Predictions from Antiquity to the Present". A Catalogue of Eclipse Cycles. Utrecht University. Retrieved 6 October 2018.

[1]

[2]

[3]

[4]

[5]

[6]

[7]

[8]

[9]

[10]

[11]

[12]