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    1. http://www.stsci.edu/ops/swat/safing/95008/93-4.txt
    ... the solar arrays could rotate before excessive array rotation is detected and halted by the solar array rotation safing check ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ops/swat/safing/95008/93-4.txt -- 19.6 Кб -- 11.01.1995
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    2. http://www.stsci.edu/spst/lrpg/documentation/procedures/lrpg_orbit_model_plus_constraint_set.html
    ... are not critical for the primary purpose of this procedure, but as an example, the second tab shows the altitude decay rate which varies with phase of the 22-year solar cycle, solar rotation, short-term solar activity, and Earth's atmospheric response ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/spst/lrpg/documentation/procedures/lrpg_orbit_model_plus_constraint_set.html -- 7.9 Кб -- 23.03.2011
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    3. Additional DF-224 Processing
    ... Additional DF-224 Processing . Pointing Control . Solar Array rotations . High Gain Antenna pointing . Electrical Power System . ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/hst/training/events/HowHSTWorks/SSD990225/tsld021.htm -- 2.4 Кб -- 23.12.2007
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    4. http://www.stsci.edu/institute/conference/iausps13/SpS13_program_0508.pdf
    ... Solar-type physics and solar-type stars II Improving our understanding of solar physics by studying other stars Helium in solar-type stars Rotation and differential rotation in solar-type stars Session W3 20+10 20+10 20+10 10+5 10+5 Wednesday, 16:00 - 18 ...
    [ Текст ]  Ссылки http://www.stsci.edu/institute/conference/iausps13/SpS13_program_0508.pdf -- 167.4 Кб -- 05.02.2013
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    5. http://www.stsci.edu/institute/conference/iausps13/presentations/SpS13_program_0810.pdf
    ... Solar-like oscillations in intermediate-mass stars Intermediate-mass stars: magnetic fields, rapid rotation, and seismology A ...
    [ Текст ]  Ссылки http://www.stsci.edu/institute/conference/iausps13/presentations/SpS13_program_0810.pdf -- 162.9 Кб -- 05.02.2013
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    6. HST Primer for Cycle 22
    ... As shown in Figure 2.1 , U1 lies along the optical axis, U2 is parallel to the solar array rotation axis, and U3 is perpendicular to the solar array axis. ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/hst/hst/proposing/documents/primer/Ch_2_Systemoverview2.html -- 20.7 Кб -- 12.04.2016
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    7. Conferences at the Institute
    ... Lucianne Walkowicz - Rotation and differential rotation in solar-type stars . Werner Weiss - BRITE - Constellation . ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/institute/conference/iausps13/presentations -- 14.6 Кб -- 11.04.2016
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    8. http://www.stsci.edu/ftp/observing/status_reports/old_reports_97/hst_status_04_01_97
    ... The solar array rotate command was issued = at 090/233920Z, and the solar array slew and type 2 slew command were = issued at 090/233941Z. At 090/234112Z the minus wing failed the SADE = torque test and the HST entered software sun point. ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/ftp/observing/status_reports/old_reports_97/hst_status_04_01_97 -- 7.6 Кб -- 01.04.1997
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    9. IAU Symposium 258 Poster Abstracts
    ... We have conducted global-scale fully 3-D MHD simulations of convection in more rapidly rotating solar-type stars with the ASH code, exploring the effects of more rapid rotation on stellar convection and the resulting magnetic dynamo action. ...
    [ Сохраненная копия ]  Ссылки http://www.stsci.edu/institute/conference/iau258/posters -- 105.2 Кб -- 10.04.2016
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    10. http://www.stsci.edu/institute/conference/iausps13/presentations/Maehara.pdf
    ... e.g. rotation period Flares on solar-type stars Supreflares on solar-type stars are difficult to observe because.. ...
    [ Текст ]  Ссылки http://www.stsci.edu/institute/conference/iausps13/presentations/Maehara.pdf -- 1529.0 Кб -- 05.02.2013
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