https://sprg.ssl.berkeley.edu/~tohban/wiki/index.php?title=Edward_Chupp&feed=atom&action=historyEdward Chupp - Revision history2024-03-28T11:42:49ZRevision history for this page on the wikiMediaWiki 1.16.0https://sprg.ssl.berkeley.edu/~tohban/wiki/index.php?title=Edward_Chupp&diff=10782&oldid=prevSchriste at 19:00, 22 August 20182018-08-22T19:00:37Z<p></p>
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<tr><td class='diff-marker'>-</td><td style="background: #ffa; color:black; font-size: smaller;"><div>|next_nugget = [<del class="diffchange diffchange-inline">http</del>:<del class="diffchange diffchange-inline">//sprg.ssl.berkeley.edu/~tohban/wiki/index.php/Radio_Emissions_from_Double_RHESSI_TGFs Terrestrial gamma rays</del>]</div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div>|next_nugget=<ins class="diffchange diffchange-inline">{{#ask: [</ins>[<ins class="diffchange diffchange-inline">Category</ins>:<ins class="diffchange diffchange-inline">Nugget</ins>]<ins class="diffchange diffchange-inline">] [[RHESSI Nugget Index::295]]}}</ins></div></td></tr>
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</table>Schristehttps://sprg.ssl.berkeley.edu/~tohban/wiki/index.php?title=Edward_Chupp&diff=9607&oldid=prevHhudson at 13:25, 14 March 20172017-03-14T13:25:07Z<p></p>
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<tr><td class='diff-marker'>-</td><td style="background: #ffa; color:black; font-size: smaller;"><div>|next_nugget = Terrestrial gamma rays</div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div>|next_nugget = <ins class="diffchange diffchange-inline">[http://sprg.ssl.berkeley.edu/~tohban/wiki/index.php/Radio_Emissions_from_Double_RHESSI_TGFs </ins>Terrestrial gamma rays<ins class="diffchange diffchange-inline">]</ins></div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>|previous_nugget = [http://sprg.ssl.berkeley.edu/~tohban/wiki/index.php/Pierre_Kaufmann Pierre Kaufmann] </div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>|previous_nugget = [http://sprg.ssl.berkeley.edu/~tohban/wiki/index.php/Pierre_Kaufmann Pierre Kaufmann] </div></td></tr>
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</table>Hhudsonhttps://sprg.ssl.berkeley.edu/~tohban/wiki/index.php?title=Edward_Chupp&diff=9583&oldid=prevHhudson: links2017-03-06T18:42:21Z<p>links</p>
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<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>Ed is best known for his pioneering work in gamma-ray astronomy with both balloon-borne and satellite instruments starting in the 1960s. </div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>Ed is best known for his pioneering work in gamma-ray astronomy with both balloon-borne and satellite instruments starting in the 1960s. </div></td></tr>
<tr><td class='diff-marker'>-</td><td style="background: #ffa; color:black; font-size: smaller;"><div>He was Principal Investigator for the gamma-ray spectrometers on the “Orbiting Solar Observatory” OSO 7 <del class="diffchange diffchange-inline">(OSO H)</del>, which flew from 1971-1974, </div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div>He was Principal Investigator for the gamma-ray spectrometers on the “Orbiting Solar Observatory” <ins class="diffchange diffchange-inline">[https://en.wikipedia.org/wiki/OSO_7 </ins>OSO 7<ins class="diffchange diffchange-inline">]</ins>, which flew from 1971-1974, </div></td></tr>
<tr><td class='diff-marker'>-</td><td style="background: #ffa; color:black; font-size: smaller;"><div>and on the Solar Maximum Mission from 1980 to 1989. </div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div>and on the <ins class="diffchange diffchange-inline">[https://en.wikipedia.org/wiki/Solar_Maximum_Mission </ins>Solar Maximum Mission<ins class="diffchange diffchange-inline">] </ins>from 1980 to 1989. </div></td></tr>
<tr><td class='diff-marker'>-</td><td style="background: #ffa; color:black; font-size: smaller;"><div>He made many discoveries with these instruments, including the first cosmic detection of gamma rays from nuclear reactions during solar flares in 1972, </div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div>He made many discoveries with these instruments, including the first cosmic detection of gamma rays from nuclear reactions during solar flares in 1972 <ins class="diffchange diffchange-inline">(Ref. [1])</ins>, </div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>the first detection of positrons at the Sun via their annihilation radiation, and the first observation of gamma rays from pulsars. </div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>the first detection of positrons at the Sun via their annihilation radiation, and the first observation of gamma rays from pulsars. </div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>The field of gamma-ray astronomy, founded on many of his seminal contributions, has blossomed into an essential window into the cosmos </div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>The field of gamma-ray astronomy, founded on many of his seminal contributions, has blossomed into an essential window into the cosmos </div></td></tr>
<tr><td class='diff-marker'>-</td><td style="background: #ffa; color:black; font-size: smaller;"><div>summarized in his 1976 book entitled “Gamma Ray Astronomy (Nuclear Transition Region)<del class="diffchange diffchange-inline">.</del>” </div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div>summarized in his 1976 book entitled “Gamma Ray Astronomy (Nuclear Transition Region)” <ins class="diffchange diffchange-inline">(Ref. [2]) </ins></div></td></tr>
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<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>=== References ===</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>=== References ===</div></td></tr>
</table>Hhudsonhttps://sprg.ssl.berkeley.edu/~tohban/wiki/index.php?title=Edward_Chupp&diff=9555&oldid=prevHhudson at 15:31, 3 March 20172017-03-03T15:31:44Z<p></p>
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<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>Ed got an AB with Honors in Physics in 1950 and his PhD in 1954, both from the University of California, Berkeley. </div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>Ed got an AB with Honors in Physics in 1950 and his PhD in 1954, both from the University of California, Berkeley. </div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>For his research there, he worked on detecting radiation from space, and placed one of the first high-altitude neutron monitors on the Mauna Kea volcano in Hawaii. </div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>For his research there, he worked on detecting radiation from space, and placed one of the first high-altitude neutron monitors on the Mauna Kea volcano in Hawaii. </div></td></tr>
<tr><td class='diff-marker'>-</td><td style="background: #ffa; color:black; font-size: smaller;"><div>He was a staff scientist at <del class="diffchange diffchange-inline">Livermore National </del>Laboratory from 1954 until 1959, Chief of the Geophysics Division at Boeing Aerospace from 1959-1962, </div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div>He was a staff scientist at <ins class="diffchange diffchange-inline">the University of California Radiation </ins>Laboratory <ins class="diffchange diffchange-inline">at Livermore </ins>from 1954 until 1959, Chief of the Geophysics Division at Boeing Aerospace from 1959-1962, </div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>and a Professor at the University of New Hampshire from 1962 until his retirement in 2007. </div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>and a Professor at the University of New Hampshire from 1962 until his retirement in 2007. </div></td></tr>
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</table>Hhudsonhttps://sprg.ssl.berkeley.edu/~tohban/wiki/index.php?title=Edward_Chupp&diff=9553&oldid=prevBdennis: Minor edit2017-03-03T14:39:41Z<p>Minor edit</p>
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<tr><td class='diff-marker'>-</td><td style="background: #ffa; color:black; font-size: smaller;"><div>RHESSI has lost another good friend, <del class="diffchange diffchange-inline"> </del>the creator of the field of solar gamma-ray astronomy.</div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div>RHESSI has lost another good friend, the creator of the field of solar gamma-ray astronomy.</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>Ed got an AB with Honors in Physics in 1950 and his PhD in 1954, both from the University of California, Berkeley. </div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>Ed got an AB with Honors in Physics in 1950 and his PhD in 1954, both from the University of California, Berkeley. </div></td></tr>
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<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>and on the Solar Maximum Mission from 1980 to 1989. </div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>and on the Solar Maximum Mission from 1980 to 1989. </div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>He made many discoveries with these instruments, including the first cosmic detection of gamma rays from nuclear reactions during solar flares in 1972, </div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>He made many discoveries with these instruments, including the first cosmic detection of gamma rays from nuclear reactions during solar flares in 1972, </div></td></tr>
<tr><td class='diff-marker'>-</td><td style="background: #ffa; color:black; font-size: smaller;"><div>the first detection positrons at the Sun via their annihilation radiation, and the first observation of gamma rays from pulsars. </div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div>the first detection <ins class="diffchange diffchange-inline">of </ins>positrons at the Sun via their annihilation radiation, and the first observation of gamma rays from pulsars. </div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>The field of gamma-ray astronomy, founded on many of his seminal contributions, has blossomed into an essential window into the cosmos </div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>The field of gamma-ray astronomy, founded on many of his seminal contributions, has blossomed into an essential window into the cosmos </div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>summarized in his 1976 book entitled “Gamma Ray Astronomy (Nuclear Transition Region).” </div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>summarized in his 1976 book entitled “Gamma Ray Astronomy (Nuclear Transition Region).” </div></td></tr>
</table>Bdennishttps://sprg.ssl.berkeley.edu/~tohban/wiki/index.php?title=Edward_Chupp&diff=9552&oldid=prevHhudson at 14:15, 3 March 20172017-03-03T14:15:10Z<p></p>
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</table>Hhudsonhttps://sprg.ssl.berkeley.edu/~tohban/wiki/index.php?title=Edward_Chupp&diff=9551&oldid=prevHhudson: added links and polished a bit2017-03-03T14:13:33Z<p>added links and polished a bit</p>
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<tr><td class='diff-marker'>-</td><td style="background: #ffa; color:black; font-size: smaller;"><div>RHESSI has lost another good friend <del class="diffchange diffchange-inline">who initiated </del>the field of solar gamma-ray astronomy.</div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div>RHESSI has lost another good friend<ins class="diffchange diffchange-inline">, the creator of </ins>the field of solar gamma-ray astronomy.</div></td></tr>
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<tr><td class='diff-marker'>-</td><td style="background: #ffa; color:black; font-size: smaller;"><div>Ed got an AB with Honors in Physics in 1950 and his PhD in 1954, both from the University of California, Berkeley. For his research there, he worked on detecting radiation from space, and placed one of the first high-altitude neutron monitors on the Mauna Kea volcano in Hawaii. He was a staff scientist at Livermore National Laboratory from 1954 until 1959, Chief of the Geophysics Division at Boeing Aerospace from 1959-1962, and a Professor at the University of New Hampshire from 1962 until his retirement in 2007. </div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div>Ed got an AB with Honors in Physics in 1950 and his PhD in 1954, both from the University of California, Berkeley. </div></td></tr>
<tr><td colspan="2"> </td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div>For his research there, he worked on detecting radiation from space, and placed one of the first high-altitude neutron monitors on the Mauna Kea volcano in Hawaii. </div></td></tr>
<tr><td colspan="2"> </td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div>He was a staff scientist at Livermore National Laboratory from 1954 until 1959, Chief of the Geophysics Division at Boeing Aerospace from 1959-1962, </div></td></tr>
<tr><td colspan="2"> </td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div>and a Professor at the University of New Hampshire from 1962 until his retirement in 2007. </div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"></td></tr>
<tr><td class='diff-marker'>-</td><td style="background: #ffa; color:black; font-size: smaller;"><div>Ed is best known for his pioneering work in gamma-ray astronomy with both balloon-borne and satellite instruments starting in the 1960s. He was Principal Investigator for the gamma-ray spectrometers on the “Orbiting Solar Observatory” OSO 7 (OSO H), which flew from 1971-1974, and the Solar Maximum Mission from 1980 to 1989. He made many discoveries with these instruments including the first cosmic detection of gamma rays from nuclear reactions during solar flares in 1972, the detection <del class="diffchange diffchange-inline">of </del>the annihilation <del class="diffchange diffchange-inline">of positrons</del>, and the <del class="diffchange diffchange-inline">discovery </del>of gamma rays from pulsars. The field of gamma-ray astronomy, founded on many of his seminal contributions, has blossomed into an essential window into the cosmos summarized in his 1976 book entitled “Gamma Ray Astronomy (Nuclear Transition Region).” </div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div>Ed is best known for his pioneering work in gamma-ray astronomy with both balloon-borne and satellite instruments starting in the 1960s. </div></td></tr>
<tr><td colspan="2"> </td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div>He was Principal Investigator for the gamma-ray spectrometers on the “Orbiting Solar Observatory” OSO 7 (OSO H), which flew from 1971-1974, </div></td></tr>
<tr><td colspan="2"> </td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div>and <ins class="diffchange diffchange-inline">on </ins>the Solar Maximum Mission from 1980 to 1989. </div></td></tr>
<tr><td colspan="2"> </td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div>He made many discoveries with these instruments<ins class="diffchange diffchange-inline">, </ins>including the first cosmic detection of gamma rays from nuclear reactions during solar flares in 1972, </div></td></tr>
<tr><td colspan="2"> </td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div>the <ins class="diffchange diffchange-inline">first </ins>detection <ins class="diffchange diffchange-inline">positrons at </ins>the <ins class="diffchange diffchange-inline">Sun via their </ins>annihilation <ins class="diffchange diffchange-inline">radiation</ins>, and the <ins class="diffchange diffchange-inline">first observation </ins>of gamma rays from pulsars. </div></td></tr>
<tr><td colspan="2"> </td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div>The field of gamma-ray astronomy, founded on many of his seminal contributions, has blossomed into an essential window into the cosmos </div></td></tr>
<tr><td colspan="2"> </td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div>summarized in his 1976 book entitled “Gamma Ray Astronomy (Nuclear Transition Region).” </div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>=== References ===</div></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"><div>=== References ===</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"></td></tr>
<tr><td class='diff-marker'>-</td><td style="background: #ffa; color:black; font-size: smaller;"><div>[1] [<del class="diffchange diffchange-inline">Chupp, E</del>.<del class="diffchange diffchange-inline">L</del>.<del class="diffchange diffchange-inline">, Forrest, D</del>.<del class="diffchange diffchange-inline">J</del>.<del class="diffchange diffchange-inline">, Higbie, P</del>.<del class="diffchange diffchange-inline">R., Suri, A.N., Tsai, C., and Dunphy, P.P. ``</del>Solar Gamma Ray Lines Observed during the Solar Activity of August 2 to August 11, 1972”<del class="diffchange diffchange-inline">, Nature, 241, 333 (1973)</del>]</div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div>[1] [<ins class="diffchange diffchange-inline">http://adsabs</ins>.<ins class="diffchange diffchange-inline">harvard</ins>.<ins class="diffchange diffchange-inline">edu/abs/1973Natur</ins>.<ins class="diffchange diffchange-inline">241</ins>..<ins class="diffchange diffchange-inline">333C "</ins>Solar Gamma Ray Lines Observed during the Solar Activity of August 2 to August 11, 1972”]</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"></td></tr>
<tr><td class='diff-marker'>-</td><td style="background: #ffa; color:black; font-size: smaller;"><div>[2] [<del class="diffchange diffchange-inline">Chupp, E</del>.<del class="diffchange diffchange-inline">L</del>. <del class="diffchange diffchange-inline">``</del>Gamma Ray Astronomy (Nuclear Transition Region)<del class="diffchange diffchange-inline">'' D. Reidel Publishing Company, Dordrecht, Holland (1976)</del>]</div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div>[2] [<ins class="diffchange diffchange-inline">http://adsabs</ins>.<ins class="diffchange diffchange-inline">harvard</ins>.<ins class="diffchange diffchange-inline">edu/abs/1976gran.book.....C "</ins>Gamma Ray Astronomy (Nuclear Transition Region)<ins class="diffchange diffchange-inline">" </ins>]</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"></td></tr>
<tr><td class='diff-marker'>-</td><td style="background: #ffa; color:black; font-size: smaller;"><div>[3] [<del class="diffchange diffchange-inline">Chupp, E</del>. <del class="diffchange diffchange-inline">L</del>.<del class="diffchange diffchange-inline">, Forrest, D</del>. <del class="diffchange diffchange-inline">J</del>.<del class="diffchange diffchange-inline">, Ryan, J</del>. <del class="diffchange diffchange-inline">M</del>.<del class="diffchange diffchange-inline">, et al</del>.<del class="diffchange diffchange-inline">, </del>“A Direct Observation of Solar Neutrons Following The 0118 UT Flare on 1980 June 21”<del class="diffchange diffchange-inline">, The Astrophysical Journal, 263, L95 (1982)</del>]</div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div>[3] [<ins class="diffchange diffchange-inline">http://adsabs</ins>.<ins class="diffchange diffchange-inline">harvard</ins>.<ins class="diffchange diffchange-inline">edu/abs/1982ApJ</ins>...<ins class="diffchange diffchange-inline">263L</ins>..<ins class="diffchange diffchange-inline">95C </ins>“A Direct Observation of Solar Neutrons Following The 0118 UT Flare on 1980 June 21”]</div></td></tr>
<tr><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"></td><td class='diff-marker'> </td><td style="background: #eee; color:black; font-size: smaller;"></td></tr>
<tr><td class='diff-marker'>-</td><td style="background: #ffa; color:black; font-size: smaller;"><div>[4] [<del class="diffchange diffchange-inline">Forrest, D</del>. <del class="diffchange diffchange-inline">J</del>.<del class="diffchange diffchange-inline">, and Chupp, E</del>.<del class="diffchange diffchange-inline">, </del> “Simultaneous acceleration of electrons and Ions in solar flares”<del class="diffchange diffchange-inline">, Nature, 305, 291 (1983)</del>]</div></td><td class='diff-marker'>+</td><td style="background: #cfc; color:black; font-size: smaller;"><div>[4] [<ins class="diffchange diffchange-inline">http://adsabs</ins>.<ins class="diffchange diffchange-inline">harvard</ins>.<ins class="diffchange diffchange-inline">edu/abs/1983Natur</ins>.<ins class="diffchange diffchange-inline">305..291F </ins> “Simultaneous acceleration of electrons and Ions in solar flares”]</div></td></tr>
</table>Hhudsonhttps://sprg.ssl.berkeley.edu/~tohban/wiki/index.php?title=Edward_Chupp&diff=9547&oldid=prevBdennis: Initital draft2017-03-02T22:49:28Z<p>Initital draft</p>
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|title = Edward Chupp<br />
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|publish_date = 06 March 2017<br />
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[[File:EdChupp.jpg|500px|thumb|center| <br />
Edward L. Chupp, deceased February 21st, 2017, at the age of 89.<br />
]]<br />
<br />
RHESSI has lost another good friend who initiated the field of solar gamma-ray astronomy.<br />
<br />
Ed got an AB with Honors in Physics in 1950 and his PhD in 1954, both from the University of California, Berkeley. For his research there, he worked on detecting radiation from space, and placed one of the first high-altitude neutron monitors on the Mauna Kea volcano in Hawaii. He was a staff scientist at Livermore National Laboratory from 1954 until 1959, Chief of the Geophysics Division at Boeing Aerospace from 1959-1962, and a Professor at the University of New Hampshire from 1962 until his retirement in 2007. <br />
<br />
Ed is best known for his pioneering work in gamma-ray astronomy with both balloon-borne and satellite instruments starting in the 1960s. He was Principal Investigator for the gamma-ray spectrometers on the “Orbiting Solar Observatory” OSO 7 (OSO H), which flew from 1971-1974, and the Solar Maximum Mission from 1980 to 1989. He made many discoveries with these instruments including the first cosmic detection of gamma rays from nuclear reactions during solar flares in 1972, the detection of the annihilation of positrons, and the discovery of gamma rays from pulsars. The field of gamma-ray astronomy, founded on many of his seminal contributions, has blossomed into an essential window into the cosmos summarized in his 1976 book entitled “Gamma Ray Astronomy (Nuclear Transition Region).” <br />
<br />
=== References ===<br />
<br />
[1] [Chupp, E.L., Forrest, D.J., Higbie, P.R., Suri, A.N., Tsai, C., and Dunphy, P.P. ``Solar Gamma Ray Lines Observed during the Solar Activity of August 2 to August 11, 1972”, Nature, 241, 333 (1973)]<br />
<br />
[2] [Chupp, E.L. ``Gamma Ray Astronomy (Nuclear Transition Region)'' D. Reidel Publishing Company, Dordrecht, Holland (1976)]<br />
<br />
[3] [Chupp, E. L., Forrest, D. J., Ryan, J. M., et al., “A Direct Observation of Solar Neutrons Following The 0118 UT Flare on 1980 June 21”, The Astrophysical Journal, 263, L95 (1982)]<br />
<br />
[4] [Forrest, D. J., and Chupp, E., “Simultaneous acceleration of electrons and Ions in solar flares”, Nature, 305, 291 (1983)]</div>Bdennis