1 / 30

SUN COURSE - SLIDE SHOW 3

SUN COURSE - SLIDE SHOW 3. Show 1 -- photosphere & sunspots. Today: SOHO. Show 2 -- corona & solar cycle. 1. SOHO (Solar & Heliospheric Observatory). Computer animation of trip to orbit 1% of distance to Sun New collaborative ESA/NASA mission - launched Dec 1995

ayita
Télécharger la présentation

SUN COURSE - SLIDE SHOW 3

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript


  1. SUN COURSE - SLIDE SHOW 3 Show 1 -- photosphere & sunspots Today: SOHO Show 2 -- corona & solar cycle

  2. 1. SOHO (Solar & Heliospheric Observatory) Computer animation of trip to orbit 1% of distance to Sun New collaborative ESA/NASA mission - launched Dec 1995 --> 1st comprehensive view of Sun

  3. SOHO Orbit Orbiting Sun at L1 point in phase with Earth Observing Sun continuously for first time Results breathtaking MANY NEW SURPRISES --> only three

  4. Suite 11 Instrument Packages Solar wind - SWAN, CELIAS, CEPAC Atmosphere: * LASCO - Visible Light Coronagraph - UVCS - Ultraviolet Coronagraph - * EIT - Extreme UV telescope - global images- CDS - Spectrum EUV -> n, T, v + raster SUMER - Spectrum EUV -> n, T, v + raster Interior * MDI - Oscillations Imager + B GOLF - Global Velocity Oscillations * VIRGO - Irradiance Variations

  5. E.G. from CDS

  6. The SUN Last Week The photo sphere (Big Bear)

  7. The SUN TODAY The photo sphere (SOHO-MDI)

  8. Magnetic field(SOHO-MDI)

  9. Chromosphere (Ha - Big Bear)

  10. Chromosphere (CaK - Big Bear)

  11. Chromosphere (SOHO-EIT)

  12. Corona at 1.3 MK(EIT)

  13. Corona at 1.6 MK(EIT)

  14. Corona at 2.3 MK(EIT)

  15. 2. QNs. (i) -- ? Earth Influenced by S Variability Number of Sunspots Oscillates w. 11-year Cycle

  16. SURPRISE (1976) Realised NO sunspots in most of 17th centy "Maunder Minimum" -- Little Ice Age So B on Sun affects climate of Earth !! How ??

  17. SOHO --> Total Emission (t) 1996-2000 Emission varies by 0.2% -- passage sunspots Increase by 0.1% from sunspot min to max ? Contribution to global warming

  18. SURPRISE (2001) Discovered that Global B of Sun doubled since 1900 ? Effect on Global T of Earth Observed increase in T (blue) Best estimate of increase caused by Sun (yellow) Only 1/3 global warming (1970 to 2000) caused by Sun ? Mechanism couple Sun/climate

  19. QN. (ii) -- ? Structure of Solar Interior Guitar string can oscillate in different normal modes Sun too Recently discovered several million

  20. SOHO Measures velocity of Sun's surface at million pts/min Deduces frequencies: Deduced T(r) -- agrees with model to < 1%

  21. Deduce Internal Rotation Observe: * Faster at equator -- Expect: * const. on cylinders * B generated throughout conv. zone Surprise: -- const on radial lines -- intense shear layer ? site dynamo

  22. QN(iii)-? How Do Mass Ejections Occur SOHO Coronagraph -- Artificial eclipse Discovered huge ejections of plasma Can reach Earth - communications / satellites

  23. Comet + Comet

  24. Next

  25. TODAY - SOHO LASCO Corona-graph

  26. Further Out (LASCO C3)

  27. ? Effect on the Earth -- Space Weather

  28. Other Consequences Damage to satellites, astronauts Disruption to radio/phone communications, power grids

  29. Cause of Eruption Magnetic Catastrophe (2D)

  30. 3D Model Magnetic Catastrophe

More Related