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--- main:related_info [2014/02/10 22:23]
bruce created
+++ main:related_info [2021/01/12 00:50] (current)
@@ Line 1: / Line 1: @@
-<UL>
+====== General GRB-Related Information ======
-   <li>Other Instruments</li>
-== Space Environment==
+----
- <li>Particle & CR Environment and Issues</li>
+====== Other Instruments ======
+You can find information on Scheduled Space Launches on this page:
+http://www.satelliteonthenet.co.uk/index.php/2015
-<table border="1">
-<tr><td><b>Document Name+Link</b></td><td><b>Date</b></td><td><b>Type (1)</b></td><td><b>Author</b></td><td><b>Comment</b></td><td> <b>Keywords</b></td></tr>
+====== Space Environment ======
-<tr><td>Reference on Space Particle Environment
-[[Media:stassinopoulos.pdf]]
-</td><td>?</td><td>?</td><td>stassinopoulos</td><td>Particle Background and Environment Data </td><td>Particle background, latitude, SAA, electron population, particle contours, high background region, map of radiation belts, van allen belts</td></tr>
+===== Particle & CR Environment and Issues =====
+^Document Name+Link^Date^Type^Author^Comment^Keywords^
+|"World Maps of Constant B, L, and Flux Contours", E. G. Stassinopoulos, NASA SP-3054, Goddard Space Flight Center, 1970 {{:main:stassinopoulos_earth_mag_field_particles.pdf|stassinopoulos.pdf}} |1970|NASA Report|Stassinopoulos|Reference on Space Particle Environment|Particle background, latitude, SAA, electron population, particle contours, high background region, map of radiation belts, van allen belts, cutoff of rigidity,COR|
-<tr><td>Next Item  </td><td>Next Date</td><td>Next Type</td><td>Next Author</td><td>Next Comment</td><td> Next Keywordt</td></tr>
-</table>
+====== Cosmic Backgrounds ======
+===== X-ray =====
+===== UV background =====
+ is given in [[Media:1987AJ_____94__876O.pdf]]
+===== Optical-IR background =====
-<li>Cosmic Backgrounds</li>
- <UL>
-  <li>X-ray</li>
-<li>The UV background is given in [[Media:1987AJ_____94__876O.pdf]]</li>
-<li> optical-IR</li>
 My favorite plot of space (zodiacal) background opt-NIR is the one by Michael Lampton (though I think aldering's analysis below is better:
-[[File:lampton_space_bgnd.png]]
+{{ :main:lampton_space_bgnd.png?direct&300 |lampton_space_bgnd.png}}
-I believe you can take as definitive Greg Aldering's analysis of space background for SNAP [[Media:aldering01_space_zodi.pdf]]. DO NOT USE without attribution!!! (called the "white paper" elsewhere, probably a section of, or a study for the white paper; the original file was just called zodi.ps).
+I believe you can take as definitive Greg Aldering's analysis of space background for SNAP {{:main:aldering01_space_zodi.pdf|aldering01_space_zodi.pdf}} DO NOT USE without attribution!!! (called the "white paper" elsewhere, probably a section of, or a study for the white paper; the original file was just called zodi.ps).
 It is important to understand that the zodi varies depending on angle between sun and pointing.  I *think* in the optical it doesn't vary so much, but don't quote me on that.
@@ Line 43: / Line 44: @@
 </ul>
+====== Lya Forest Spectroscopy ======
+Of interest because high-z grb may provide very bright light sources for very high-z Lyman Alpha Forests.
+Some papers to check out some day:
+http://arxiv.org/abs/1309.1477v1      Observational Requirements for Lyman-alpha Forest Tomographic Mapping of Large-Scale Structure at z ~ 2

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