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101. Filming The Sun CML-Cinematography Mailing List
The Cinematography mailing List CML is sponsored by - When I studiedastrophysics at the University of Arizona, we used very specialized filters on
http://www.cinematography.net/Pages GB/[cml] Shooting the Sun.htm
The Cinematography Mailing List - CML is sponsored by :-
kweiwss(kwei[2],"slidesc","sponsorsc",1); kweisi(kwei[2],"slidesc","r"); // kwei [9] [slidesc] [sponsorsc] kweiwss(kwei[3],"slidesd","sponsorsd",1); kweisi(kwei[3],"slidesd","r"); // kwei [9] [slidesd] [sponsorsd] kweiwss(kwei[4],"slidese","sponsorse",1); kweisi(kwei[4],"slidese","r"); // kwei [9] [slidese] [sponsorse] kweiwss(kwei[1],"slidesb","sponsorsb",1); kweisi(kwei[1],"slidesb","r"); // kwei [9] [slidesb] [sponsorsb] kweiwss(kwei[0],"slidesa","sponsorsa",1); kweisi(kwei[0],"slidesa","r"); // kwei [9] [slidesa] [sponsorsa]
document.write(doClock("W0","%20-%20","M0","%20-%20","D1","%20-%20","Y0"));

do not use without permission
Filming The Sun
Yours, Exposure is only one of the things you need to address. if you are shooting at ~1/30th, good starting point would be somwhere around f256 for 200 ISO film. Obviously, you Another element that would seem to be of likely concern is to be able to get some color to the sun. If you shoot this sun mid-day, as your discription calls for, you will get nothing but a white disc. You will need to add color, if you want color. Yet another element to be concerned with is whether you want to make allowances for how people have come to view "big sun" photographs. Most people have an association that has them prejudiced twards a sun that shimmers. This shimmering they've seen in previous photography comes from atmospheric interferance when shooting the sun low on the horizon. If you want this effect, shoot the sun close to the horizon, but since it is to be a mid afternoon sun, be certain to not include any horizon. The closer you shoot the sun to the horizon the less color filtration you will need ... a "rosey sunset" is caused by the filtration of the sun's light through the atmosphere on earth.

102. Astronomy & Astrophysics Resources -- Arts & Sciences Libraries, UB Libraries
Here are resources related to astronomy and astrophysics at the Science and Below is a list of selected Internet resources for Astronomy organized by
http://ublib.buffalo.edu/libraries/asl/guides/astronomy.html
Below is a list of selected Internet resources for Astronomy organized by type of information source. For more information on Astronomy, visit the Physics Department here at the State University of New York at Buffalo. Acronyms used on this page NASA (National Aeronautics and Space Administration (U.S.)); NRAO (National Radio Astronomy Observatory (U.S.)) Career Information News and Discussion Lists
  • Sedna Planetary Information and News Pages
    • NASA News Start here. Additional pages include:

103. Marxism Message, [Marxism] Natural Scientists Protest Misuse Of Science
Below is a list of prominent signatories of the UCS RSI statement. Laboratory_ Marxism mailing list
http://archives.econ.utah.edu/archives/marxism/2004w07/msg00282.htm
Marxism
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[Marxism] Natural Scientists protest misuse of science
  • To : "Marxmail List" < Subject : [Marxism] Natural Scientists protest misuse of science From : "Jurriaan Bendien" < Date : Sun, 22 Feb 2004 07:45:39 +0100 Cc
http://www2.ucsusa.org/global_environment/rsi/rsirelease.html For more info on the campaign in defence of science, see: http://www2.ucsusa.org/global_environment/rsi/report.html http://lists.econ.utah.edu/mailman/listinfo/marxism

104. Area 51 Mailing List Digest V096.n029, 15 Dec 1996
Area 51 mailing List Digest v096.n029 15 Dec 1996 You don t need to knowastrophysics Oh, I worked for xxxx out of Vegas, and they used to fly us in
http://www.ufomind.com/area51/list/arc/1996/v096n029.html
Area 51 Mailing List Digest v096.n029
15 Dec 1996
Index
Newsgroup Ephemera: Mom, Break-In Plan, Lazar Theory [a.c.a51] 02 - campbell@ufomind.com (Gle - Test Site Tour is filling up fast! 03 - campbell@ufomind.com (Gle - Hughes worker on Blackbird program, etc. [Anecdotal] 04 - campbell@ufomind.com (Gle - Audio Interview with Edward Teller Available on Web Transcripts of contractor who worked at A51 06 - campbell@ufomind.com (Gle - Miscellanea: Shuttle, S-4, Huachuca, U-2, Janet, etc. Possible NTS tour itinery 08 - campbell@ufomind.com (Gle - "Mars Attacks" Gave Me a Headache (nack, nack!) 09 - campbell@ufomind.com (Gle - Vatican Black Ops track Hale-Bopp object [Loon] 10 - campbell@ufomind.com (Gle - Trying to Verify Dr. Michael Wolf's foundation 11 - campbell@ufomind.com (Gle - Misc.: Local Weather, French Imagery, Shuttle, Nellis Book Archive Index Mailing List Information
Message #1
Newsgroup Ephemera: Mom, Break-In Plan, Lazar Theory [a.c.a51] my mom Breaking into area51 Lazar's theory is a bit odd? (in one big way) http://www.tiac.net/users/mayor

105. Hajime BABA, Ph.D In Astrophysics
Translate this page Hajime BABA, Ph.D in astrophysics. VSNET is a group of international mailinglists for distribution of various messages on variable stars,
http://www.kusastro.kyoto-u.ac.jp/~baba/
Department of Astronomy Kyoto University
Hajime BABA, Ph.D
Hajime BABA, Ph.D in Astrophysics
NOTE: Since April 2004, I have moved to School of Education, Waseda University as a Senior Research Associate.
Please contact to if you have any comments. This site will be moved in the near future.
Research Activities :-)
Curriculum Vitae (CV) [en] Contact information including current position, educations, employments, research interests, memberships, and publications. VSNET - our Variable Star Network [en] VSNET is a group of international mailing lists for distribution of various messages on variable stars, especially cataclysmic variables (CVs) and related objects. I'm a sub-manager of these mailing lists. SU UMa-type dwarf novae [in prep.] Dwarf novae (DNe) are a subgroup of CVs. DNe are called as " laboratory of research of accretion disk ". The SU UMa-type stars are a subgroup of DNe with the normal outbursts and superoutburst. Eclipsing cataclysmic variables [in prep.] Some binaries such as CVs show eclipses when the secondary star moves toward the front of the primary star. By analyzing these eclipse light curve, we can obtain the information about accretion disk around the primary star (i.e.: distribution of luminosity, temperature and else). Virtual Observatory (VO) [in prep.]

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