1 / 9

On the magnetic cycle in the GCR intensity in the inner and outer heliosphere

On the magnetic cycle in the GCR intensity in the inner and outer heliosphere. Topics: Near the Earth for H, T ≈ 200 MeV: J max (A<0) ≈ 0.8 J max (A<0) Beyond the TS: J max (A<0) ≈ 4 J max (A<0)? It looks so. On the causes of the magnetic cycle in the near heliosheath.

jolene-sutton
Download Presentation

On the magnetic cycle in the GCR intensity in the inner and outer heliosphere

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. On the magnetic cycle in the GCR intensity in the inner and outer heliosphere Topics: • Near the Earth for H, T≈200 MeV: Jmax(A<0) ≈ 0.8 Jmax(A<0) • Beyond the TS: Jmax(A<0) ≈4 Jmax(A<0)? It looks so. • On the causes of the magnetic cycle in the near heliosheath M.B. Krainev, M.S. Kalinin Lebedev Physical Institute, RAS, Moscow, Russia September 2008, Košice, ECRS-21

  2. The extrema of sunspot area, tilt of HCS and medium energy GCR intensity at r = 1 AU in the minima of SC 20-24 September 2008, Košice, ECRS-21

  3. The observed behavior of the GCR intensity at r = 1-105 AUin 1975-2008 September 2008, Košice, ECRS-21

  4. Composite equatorial radial profiles of the GCRintensity during minima and maximum of solar cycles September 2008, Košice, ECRS-21

  5. The normalizedsolar cycle in the GCR intensity atr=1-105AUand prediction for 2000-2012 September 2008, Košice, ECRS-21

  6. The observed behavior of the GCR intensity along with predictions for V1 September 2008, Košice, ECRS-21

  7. On the causes of the magnetic cycle in the inner heliosheath • Baranov-Malama model (IPM, RAS): Hydro-kinetic • Drifts are weak in the outer heliosheath • Electric field: ≈  to HP in the outer heliosheath; but energy changes VSW September 2008, Košice, ECRS-21

  8. On the wavy heliospheric current sheet in the 2D transport equation for the galactic cosmic rays M.B. Krainev, M.S. Kalinin Lebedev Physical Institute, RAS, Moscow, Russia Topics: • It is believed that 2D TPE only simulates CS-effects. To study them properly one needs 3D TPE. • We derive the exact 2D TPE for the intensity averaged over the longitude from the 3D one. It could be used to estimate the errors of the simulation. • We derive the expressions for the averaged over the longitude drift velocities (for any CS-surface and for the Tilted CS model) and compare them with the known ones. September 2008, Košice, ECRS-21

  9. The exact 2D TPE for intensity averaged over the longitude.The drift velocities averaged over the longitude. • 3D transport equation for U: • Averaged magnetic drift for any CS-surface (F=0): For Tilted CS-model: September 2008, Košice, ECRS-21

More Related