Cynthia Cattell

Last updated
Cynthia A. Cattell
Alma materUniversity of California, Berkeley
Scientific career
Thesis Magnetic field-aligned currents in the earth's magnetosphere  (1980)
Doctoral advisor Forrest S. Mozer

Cynthia Cattell is a space plasma physicist known for her research on solar flares and radiation belts.

Contents

Education and career

Cattell has a B.A. from Hampshire College (1974) [1] and earned her Ph.D. from the University of California, Berkeley in 1980. [2]

As of 2021, Cattell is a professor in the School of Physics and Astronomy at the University of Minnesota. [1]

Research

Cattell's research on electron holes in space helps explain the release of energy from magnetic explosions in space. [3] [4] Cattell has also examined the energization of electrons in Earth's radiation belt [5] and used satellite data to examine the behavior of ions flowing around Earth. [6] [7] Cattell uses her scientific knowledge to present the public with viewing opportunities to see the Northern Lights. [8]

Selected publications

Awards and honors

Personal life

In 2012, Cattell was diagnosed with cancer and was treated with an experimental drug developed by colleagues at University of Minnesota's Masonic Cancer Center. [13] [14] After receiving an increased dosage of an experimental drug there was a reduction in Cattell's tumor and her lymphoma was considered in remission. [15]

Related Research Articles

<span class="mw-page-title-main">Aurora</span> Atmospheric effect

An aurora , also commonly known as the northern lights or southern lights, is a natural light display in Earth's sky, predominantly seen in high-latitude regions. Auroras display dynamic patterns of brilliant lights that appear as curtains, rays, spirals, or dynamic flickers covering the entire sky.

<span class="mw-page-title-main">Coronal mass ejection</span> Ejecta from the Suns corona

A coronal mass ejection (CME) is a significant ejection of magnetic field and accompanying plasma mass from the Sun's corona into the heliosphere. CMEs are often associated with solar flares and other forms of solar activity, but a broadly accepted theoretical understanding of these relationships has not been established.

<span class="mw-page-title-main">Magnetosphere of Saturn</span> Cavity in the solar wind the sixth planet creates

The magnetosphere of Saturn is the cavity created in the flow of the solar wind by the planet's internally generated magnetic field. Discovered in 1979 by the Pioneer 11 spacecraft, Saturn's magnetosphere is the second largest of any planet in the Solar System after Jupiter. The magnetopause, the boundary between Saturn's magnetosphere and the solar wind, is located at a distance of about 20 Saturn radii from the planet's center, while its magnetotail stretches hundreds of Saturn radii behind it.

<span class="mw-page-title-main">Cluster II (spacecraft)</span> European Space Agency mission

Cluster II is a space mission of the European Space Agency, with NASA participation, to study the Earth's magnetosphere over the course of nearly two solar cycles. The mission is composed of four identical spacecraft flying in a tetrahedral formation. As a replacement for the original Cluster spacecraft which were lost in a launch failure in 1996, the four Cluster II spacecraft were successfully launched in pairs in July and August 2000 onboard two Soyuz-Fregat rockets from Baikonur, Kazakhstan. In February 2011, Cluster II celebrated 10 years of successful scientific operations in space. In February 2021, Cluster II celebrated 20 years of successful scientific operations in space. As of March 2023, its mission has been extended until September 2024. The China National Space Administration/ESA Double Star mission operated alongside Cluster II from 2004 to 2007.

<span class="mw-page-title-main">Birkeland current</span> Currents flowing along geomagnetic field lines

A Birkeland current is a set of electrical currents that flow along geomagnetic field lines connecting the Earth's magnetosphere to the Earth's high latitude ionosphere. In the Earth's magnetosphere, the currents are driven by the solar wind and interplanetary magnetic field and by bulk motions of plasma through the magnetosphere. The strength of the Birkeland currents changes with activity in the magnetosphere. Small scale variations in the upward current sheets accelerate magnetospheric electrons which, when they reach the upper atmosphere, create the Auroras Borealis and Australis.

<span class="mw-page-title-main">Magnetosphere of Jupiter</span> Cavity created in the solar wind

The magnetosphere of Jupiter is the cavity created in the solar wind by Jupiter's magnetic field. Extending up to seven million kilometers in the Sun's direction and almost to the orbit of Saturn in the opposite direction, Jupiter's magnetosphere is the largest and most powerful of any planetary magnetosphere in the Solar System, and by volume the largest known continuous structure in the Solar System after the heliosphere. Wider and flatter than the Earth's magnetosphere, Jupiter's is stronger by an order of magnitude, while its magnetic moment is roughly 18,000 times larger. The existence of Jupiter's magnetic field was first inferred from observations of radio emissions at the end of the 1950s and was directly observed by the Pioneer 10 spacecraft in 1973.

A double layer is a structure in a plasma consisting of two parallel layers of opposite electrical charge. The sheets of charge, which are not necessarily planar, produce localised excursions of electric potential, resulting in a relatively strong electric field between the layers and weaker but more extensive compensating fields outside, which restore the global potential. Ions and electrons within the double layer are accelerated, decelerated, or deflected by the electric field, depending on their direction of motion.

<span class="mw-page-title-main">Carrington Event</span> Geomagnetic storm in 1859

The Carrington Event was the most intense geomagnetic storm in recorded history, peaking on 1–2 September 1859 during solar cycle 10. It created strong auroral displays that were reported globally and caused sparking and even fires in telegraph stations. The geomagnetic storm was most likely the result of a coronal mass ejection (CME) from the Sun colliding with Earth's magnetosphere.

<span class="mw-page-title-main">Hiss (electromagnetic)</span> An electromagnetic wave phenomenon

Electromagnetic hiss is a naturally occurring Extremely Low Frequency/Very Low Frequency electromagnetic wave that is generated in the plasma of either the Earth's ionosphere or magnetosphere. Its name is derived from its incoherent, structureless spectral properties which, when played through an audio system, sound like white noise.

<span class="mw-page-title-main">Substorm</span> Short term magnetosphere disturbance

A substorm, sometimes referred to as a magnetospheric substorm or an auroral substorm, is a brief disturbance in the Earth's magnetosphere that causes energy to be released from the "tail" of the magnetosphere and injected into the high latitude ionosphere. Visually, a substorm is seen as a sudden brightening and increased movement of auroral arcs. Substorms were first described in qualitative terms by Kristian Birkeland which he called polar elementary storms. Sydney Chapman used the term substorm about 1960 which is now the standard term. The morphology of aurora during a substorm was first described by Syun-Ichi Akasofu in 1964 using data collected during the International Geophysical Year.

The Spitzer resistivity is an expression describing the electrical resistance in a plasma, which was first formulated by Lyman Spitzer in 1950. The Spitzer resistivity of a plasma decreases in proportion to the electron temperature as .

<span class="mw-page-title-main">Matt Taylor (scientist)</span> British astrophysicist (born 1973)

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<span class="mw-page-title-main">SMILE (spacecraft)</span> Chinese–European satellite studying Earths magnetosphere

Solar wind Magnetosphere Ionosphere Link Explorer (SMILE) is a planned joint venture mission between the European Space Agency and the Chinese Academy of Sciences. SMILE will image for the first time the magnetosphere of the Sun in soft X-rays and UV during up to 40 hours per orbit, improving our understanding of the dynamic interaction between the solar wind and Earth's magnetosphere. The prime science questions of the SMILE mission are

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<span class="mw-page-title-main">STEVE</span> Atmospheric optical phenomenon, which appears as a light ribbon in the sky

STEVE is an atmospheric optical phenomenon that appears as a purple and green light ribbon in the sky, named in late 2016 by aurora watchers from Alberta, Canada. According to analysis of satellite data from the European Space Agency's Swarm mission, the phenomenon is caused by a 25 km (16 mi) wide ribbon of hot plasma at an altitude of 450 km (280 mi), with a temperature of 3,000 °C and flowing at a speed of 6 km/s (3.7 mi/s). The phenomenon is not rare, but had not been investigated and described scientifically prior to that time.

Richard Mansergh Thorne was an American physicist and a distinguished professor in the department of atmospheric and oceanic sciences at UCLA. He was known for his contributions to space plasma physics. He was a fellow of the American Geophysical Union.

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James Wynne Dungey (1923–2015) was a British space scientist who was pivotal in establishing the field of space weather and made significant contributions to the fundamental understanding of plasma physics.

References

  1. 1 2 "Cynthia Cattell | School of Physics and Astronomy | College of Science and Engineering". cse.umn.edu.
  2. Cattell, Cynthia Anne (1980). Magnetic field-aligned currents in the earth's magnetosphere (Thesis).
  3. Drake, J. F.; Swisdak, M; Cattell, C.; Shay, M.A.; Rogers, B.N.; Zeiler, A. (7 February 2003). "Formation of Electron Holes and Particle Energization During Magnetic Reconnection". Science. 299 (5608): 873–877. Bibcode:2003Sci...299..873D. doi:10.1126/science.1080333. PMID   12574625. S2CID   15852390.
  4. Cattell, C. (2005). "Cluster observations of electron holes in association with magnetotail reconnection and comparison to simulations". Journal of Geophysical Research. 110 (A1): A01211. Bibcode:2005JGRA..110.1211C. doi: 10.1029/2004JA010519 . hdl: 11603/30666 .
  5. Cattell, C.; Wygant, J. R.; Goetz, K.; Kersten, K.; Kellogg, P. J.; von Rosenvinge, T.; Bale, S. D.; Roth, I.; Temerin, M.; Hudson, M. K.; Mewaldt, R. A.; Wiedenbeck, M.; Maksimovic, M.; Ergun, R.; Acuna, M.; Russell, C. T. (12 January 2008). "Discovery of very large amplitude whistler-mode waves in Earth's radiation belts" (PDF). Geophysical Research Letters. 35 (1): L01105. Bibcode:2008GeoRL..35.1105C. doi:10.1029/2007GL032009. S2CID   120148399.
  6. Baumjohann, W.; Paschmann, G.; Cattell, C. A. (1 June 1989). "Average plasma properties in the central plasma sheet". Journal of Geophysical Research: Space Physics. 94 (A6): 6597–6606. Bibcode:1989JGR....94.6597B. doi:10.1029/JA094iA06p06597.
  7. Mozer, F. S.; Cattell, C. A.; Hudson, M. K.; Lysak, R. L.; Temerin, M.; Torbert, R. B. (1980-10-01). "Satellite measurements and theories of low altitude auroral particle acceleration". Space Science Reviews. 27 (2): 155–213. Bibcode:1980SSRv...27..155M. doi:10.1007/BF00212238. ISSN   1572-9672. S2CID   122198330.
  8. Helal, Liala (January 9, 2014). "Intense northern lights may dance above Minn. tonight". MPR News. Archived from the original on 2021-07-09. Retrieved 2021-07-03.
  9. "AGU Union Fellows". Archived from the original on 2019-10-02.
  10. "APS Fellow Archive". www.aps.org.
  11. "Professor Cynthia Cattell wins Distinguished Service award | The Minnesota Supercomputing Institute". www.msi.umn.edu. Retrieved 2024-01-12.
  12. 1 2 3 "Cynthia Cattell". College of Science and Engineering. Retrieved 2024-01-12.
  13. "Donations help woman 'Tackle Cancer'". kare11.com. 29 September 2016. Retrieved 2021-07-03.
  14. "New cancer-fighting drug developed at the University of Minnesota finding early success | MHealth.org". www.mhealth.org. Retrieved 2021-07-03.
  15. "Oxis International Comments On New York Times Article About Cancer Immunotherapy :: GT Biopharma, Inc. (GTBP)". www.gtbiopharma.com. Retrieved 2021-07-03.