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    1. http://www.mso.anu.edu.au/~geoff/AGD/Winds.pdf
    ... base of the corona to millions of kilometers above the solar surface. (http://sohowww.nascom.nasa.gov/ gallery/UVCS/) Astrophysical Gas Dynamics: Stellar Winds 5/66 2.1 Hydrostatic atmospheres Analysis of the X-ray and radio emission from the solar corona ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~geoff/AGD/Winds.pdf -- 918.1 Кб -- 03.03.2016
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    2. ANU - Research School of Astronomy and Astrophysics - 5th Stromlo Symposium
    ... Disks . 1 AGN: magnetic transport; relativistic effects; powering of coronae; analogies with micro-blazars . ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/5SS/ -- 13.4 Кб -- 01.10.2012
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    3. COALA - Computational Astrophysics Laboratory
    ... We envisage that we will determine the way in which gravitational energy is channeled into the high temperature coronae of black hole accretion disks and into relativistic jets and winds. ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/coala/agn.html -- 4.4 Кб -- 01.10.2012
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    4. GSAOI Science Page
    ... Stellar population variations in star-forming regions such as Ophiuchius, Corona Australis, and Chamaeleon . ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/gsaoi/science/ -- 7.3 Кб -- 01.10.2012
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    5. RSAA Honours Courses (2006)
    ... radiative transfer, stellar model atmospheres, stellar parameters, spectral line formation, elemental abundance determinations, stellar convection, stellar winds, chromospheres, coronae, magnetic phenomena (activity, sunspots, flares, prominences etc ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/~jerjen/RSAA_Honours_Courses2006.html -- 7.6 Кб -- 01.10.2012
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    6. http://www.mso.anu.edu.au/~geoff/HEA/HEA_overview.pdf
    ... X-ray emission from the solar corona and the atmospheres of High Energy Astrophysics ... The coronae of black hole accretion discs. ... is believed to originate from a hot corona above the black hole accretion disk ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~geoff/HEA/HEA_overview.pdf -- 2636.4 Кб -- 04.03.2001
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    7. http://www.mso.anu.edu.au/5SS/Announce_2.1.pdf
    ... Microquasars and ultra-luminous X-ray sources Both 1 & 2 to include: magnetic transport; relativistic effects; coronae; high/soft and low/hard states 3. ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/5SS/Announce_2.1.pdf -- 117.3 Кб -- 13.10.2006
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    8. http://www.mso.anu.edu.au/~geoff/HEA/5_Compton_Scattering_I.pdf
    ... mc 2 T e ph High Energy Astrophysics: Compton Scattering I 56/59 Compton scattering of "soft" photons by hot thermal electrons in the coronae of accretion disks is thought to be responsible for the X-ray emission from AGN and for the X-ray emissivity of ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~geoff/HEA/5_Compton_Scattering_I.pdf -- 105.7 Кб -- 27.05.2003
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    9. http://www.mso.anu.edu.au/~geoff/AGD/Magnetic_Forces.pdf
    ... Astrophysical Gas Dynamics: Magnetic Forces 27/59 5 Sunspots Corona z B x Low magnetic field Chromosphere Sunspot region High magnetic field Sunspots are a classic example of the simple application of magnetostatics and provide us with an example of the ...
    [ Текст ]  Ссылки http://www.mso.anu.edu.au/~geoff/AGD/Magnetic_Forces.pdf -- 274.4 Кб -- 20.08.2012
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    10. RSAA Annual Report 1998
    ... From the X-ray and radio they found that optical Balmer line emission is correlated with the formation of a hard X-ray emitting corona. ...
    [ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/annualReport/1998/07_research.html -- 53.8 Кб -- 02.10.2012
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