Professional scientists are asked to send descriptions of their eclipse plans to the Working Group on Eclipses of the Solar Division of the International Astronomical Union, so that they can keep a list of observations planned. Send such descriptions, even in preliminary form, to:
International Astronomical Union
The members of the Working Group on Eclipses of the Solar Division of the IAU are: Jay M. Pasachoff (USA), Chair, Iraida S. Kim (Russia), Hiroki Kurokawa (Japan), Jagdev Singh (India), Vojtech Rusin (Slovakia), Atila Ozguc (Turkey), Fred Espenak (USA), Jay Anderson (Canada), Glenn Schneider (USA), and Michael Gill (UK).
In order to ensure that astronomers and public health authorities have access to information on safe viewing practices, the Commission on Education and Development of the IAU (the international organization for professional astronomers), set up a Solar Eclipse Education Committee. Under Prof. Jay M. Pasachoff, the Committee has assembled information on safe methods of observing the Sun and solar eclipses, eclipse-related eye injuries, and samples of educational materials on solar eclipses.
For more information, contact Prof. Jay M. Pasachoff, Hopkins Observatory, Williams College, Williamstown, Massachusetts 01267, USA (firstname.lastname@example.org). Information on safe solar filters can be obtained by contacting Dr. B. Ralph Chou (email@example.com).
The Solar Eclipse Mailing List (SEML) is an electronic news group dedicated to solar eclipses. Published by British eclipse chaser Michael Gill (firstname.lastname@example.org), it serves as a forum for discussing anything and everything about eclipses and facilitates interaction between both the professional and amateur communities.
Complete instructions are available online for subscribing and unsubscribing. Up until mid-2004, the list manager of the SEML was Patrick Poitevin (email@example.com). He maintains archives of past SEML messages through July 2004.
An international conference on solar eclipses is being planned for 2007. The main objective of the gathering is to bring together professional eclipse researchers and amateur enthusiasts in a forum conducive to the exchange of ideas, information, and plans for past and future eclipses. Previous conferences were held in Antwerp, Belgium (2000) and Milton Keynes, England (2004), the last of which had 115 delegates from 20 different countries.
The conferences are intentionally timed to coincide during years when no central eclipses occur, to avoid travel conflicts. The 2007 event is tentatively scheduled for 2007 August 24 - 26 in southern California. For more details as they become available, contact the organizers of this event (Joanne and Patrick Poitevin at firstname.lastname@example.org).
To make the NASA solar eclipse bulletins accessible to as large an audience as possible, these publications are also available via the Internet. This was made possible through the efforts and expertise of Dr. Joe Gurman (GSFC/Solar Physics Branch).
NASA eclipse bulletins can be read, or downloaded via the Internet, using a Web browser (such as Netscape/Mozilla/Firefox, Microsoft Internet Explorer, Safari, etc.) from the GSFC Solar Data Analysis Center (SDAC) Eclipse Information homepage, or from top-level Web addresses (URLs) for the currently available eclipse bulletins themselves:
Recent bulletins are available in both "html" and "pdf" format. Current plans call for making all future NASA eclipse bulletins available over the Internet, at or before publication of each. The primary goal is to make the bulletins available to as large an audience as possible, thus, some figures or maps may not be at their optimum resolution or format. Comments and suggestions are actively solicited to fix problems and improve on compatibility and formats.
Presently, the NASA eclipse bulletins are published 18 - 36 months before each eclipse, however, there have been a growing number of requests for eclipse path data with an even greater lead time. To accommodate the demand, predictions have been generated for all central solar eclipses from 1991 through 2030. All predictions are based on j = 2 ephemerides for the Sun (Newcomb 1895) and Moon (Brown 1919, and Eckert et al. 1954). The value used for the Moon's secular acceleration is n-dot= -26 arc sec/cy2 as deduced by Morrison and Ward (1975). The path coordinates are calculated with respect to the Moon's center of mass (no corrections for the Moon's center of figure). The value for ΔT (the difference between Terrestrial Dynamical Time and Universal Time is from direct measurements during the 20th century and extrapolation into the 21st century. The value used for the Moon's mean radius is k = 0.272281.
The umbral path characteristics have been predicted with a 1 min time interval compared to the 6 min interval used in Fifty Year Canon of Solar Eclipses: 1986 - 2035 (Espenak 1987). This provides enough detail for making preliminary plots of the path on larger scale maps. Global maps using an orthographic projection also present the regions of partial and total (or annular) eclipse. Path tables and maps for these eclipses can be found on a special Website.
A special Web site has been set up to supplement this bulletin with additional predictions, tables, and data for the total solar eclipse of 2006. Some of the data posted there include an expanded version of Tables 7 and 8 (Mapping Coordinates for the Zones of Grazing Eclipse), and local circumstance tables with additional cities, as well as for astronomical observatories. Also featured will be higher resolution maps of selected sections of the path of totality and limb profile figures for other locations/times along the path.
This publication provides comprehensive information on the 2006 total solar eclipse to both the professional, and amateur and lay communities. Certain investigations and eclipse experiment, however, may require additional information which lies beyond the scope of this work. The authors invite the international professional community to contact them for assistance with any aspect of eclipse prediction including predictions for locations not included in this publication, or for more detailed predictions for a specific location (e.g., lunar limb profiles and limb-corrected contact time for an observing site.
This service is offered for the 2006 eclipse, as well as for previous eclipses in which analysis is still in progress. To discuss individual needs and requirements, please contact Fred Espenak (email@example.com).
Algorithms for the eclipse predictions were developed by Espenak primarily from the Explanatory Supplement (1974) with additional algorithms from Meeus et al. (1966) and Meeus (1982). The solar and lunar ephemerides were generated from the JPL DE200 and LE200, respectively. All eclipse calculations were made using a value for the Moon's radius of k = 0.2722810 for umbral contacts, and k = 0.2725076 (adopted IAU value) for penumbral contacts. Center of mass coordinates were used except where noted. Extrapolating from 2004 to 2006, a value for ΔT of 64.9 s was used to convert the predictions from Terrestrial Dynamical Time to Universal Time The international convention of presenting date and time in descending order has been used throughout the bulletin (i.e., year, month, day, hour, minute, second).
The primary source for geographic coordinates used in the local circumstances tables is The New International Atlas (Rand McNally 1991). Elevations for major cities were taken from Climates of the World (U.S. Dept. of Commerce 1972). The names and spellings of countries, cities, and other geopolitical regions are not authoritative nor do they imply any official recognition in status. Corrections to names, geographic coordinates, and elevations are actively solicited in order to update the database for future eclipse bulletins.