|
|
Click the serial number on the left to view the details of the item. |
# |
Author | Title | Accn# | Year | Item Type | Claims |
1 |
Howe, R. (ed.) |
Subsurface and atmospheric influences on solar activity : Proceedings of the 24th National Solar Observatory Sacramento Peak wor |
022001 |
2008 |
Book |
|
2 |
B. Schmieder (ed.) |
Third advances in solar physics euroconference : Magnetic fields and oscillations : Proc. of a meeting held in Potsdam/Caputh, G |
016533 |
1999 |
Book |
|
|
1.
|
|
Title | Subsurface and atmospheric influences on solar activity : Proceedings of the 24th National Solar Observatory Sacramento Peak workshop held from April 16-20, 2007 at the National Solar Observatory/Sacramento Peak, Sunspot, New Mexico, USA |
Author(s) | Howe, R. (ed.);Komm, R.W. (ed.);Balasubramaniam, K.S. (ed.);Petrie, G.J.D. (ed.) |
Publication | California, USA, Astronomical Society of the Pacific, 2008. |
Description | xiv, 440p. |
Series | (Astronomical Society of the Pacific Conference Series) |
Abstract Note | The 24th NSO Workshop focused on solar active regions, their origin and evolution on the sun inferred from helioseismology, magnetometry and modeling. The combination of helioseismic, observational and theoretical efforts makes it possible, for example, to follow twist and helicity of magnetic fields/flux tubes from below the solar surface through the solar atmosphere into the interplanetary medium. Helicity-loaded fields are very probably responsible for the most geoeffective solar phenomena such as coronal mass ejections and flares. The main aim of this workshop was to bring together experts in magnetometry, activity, and helioseismology, to further our understanding of solar active regions and their creation and evolution.
The 1 keynote, 12 invited and 27 contributed talks as well as 9 posters combined to provide an overview of the understanding of solar active regions. The key topics for this meeting were flows around active regions: surface and below, flux emergence and cancellation, space weather and active regions: back to front, morphology of active regions and filaments, magnetic flux and magneto-acoustic waves, and influences on coronal complexity.
This book is suitable for researchers and graduate students
|
ISBN,Price | 9781583813294 : US$ 77.00 |
Classification | 520/524(069)
|
Keyword(s) | 1. HELIOSEISMOLOGY - PROC.
2. MAGNETOMETRY - PROC.
3. NATIONAL SOLAR OBSERVATORY WORKSHOP; 024
|
Item Type | Book |
Circulation Data
Accession# | |
Call# | Status | Issued To | Return Due On | Physical Location |
022001 |
|
520/524(069)/A.S.P.C.S./022001 |
On Shelf |
|
|
|
+Copy Specific Information | |