Preface
Preface
The CNRS astrophysics schools gather professional astronomers several times per
year to discuss hot scientific topics. Since 2003 and every 3 years, at Oléron and
then at La Rochelle, a CNRS astrophysics school welcomes, for the first time,
amateur astronomers. That is how about 15 professionals and 35 amateurs, with
already a good practice of astronomy, meet to exchange on topics and methods of
observations. The goal is to have the passion for astronomy of amateurs converge
with useful objectives for the scientific community.
This book is the result of lectures given during the first CNRS school gathering
professional and amateur astronomers, held in Oléron (France) from May 6 to 11,
2003, and which was entitled1 :
“Outils de l’astrophysique pour une coopération entre astronomes professionnels et
amateurs.”
During this meeting the contribution of professional to amateur work was mainly
focused towards observing techniques, various possible common programmes or
studies, scientific resources and methodology. The school was particularly focused
on spectroscopy, a method to analyse light which allows a better knowledge of the
physics of astronomical bodies. A cornerstone of professional astrophysics, spectroscopy now tends to develop among amateurs.
The goal of professional-amateur schools is to guide amateurs by proposing on
one hand an update on astrophysics and on the knowledge of professional scientific
needs, and on the other hand to define together a methodology for observing programmes. Moreover, professionals can realize during these schools what amateurs
can bring to their studies and propose federative scientific programmes.1
Indeed, in spite of the means put together by professionals, with an increasing complexity, the sky remains vast. A number of observations can be executed
by amateurs with small instruments and become part of larger professional campaigns. Compared to powerful professional telescopes, the instruments of amateurs
are of course modest, but they have recording and measuring equipments with the
same technology as professionals. In addition, size is not always a handicap if
the observations are frequent and regularly scheduled. Finally, amateurs have a
much bigger reactivity to follow a sudden and unexpected astronomical event than
professionals who have to follow a long procedure before pointing a telescope to a
chosen object.
Nowadays a large number of amateur astronomers are equipped with an instrumentation allowing to produce measurements likely to interest the community of
professional astronomers. In particular, the use of CCD cameras has widely spread
1 See
http://www.astrosurf.com/aude/oleron
IV
among amateurs and opened the road to already fruitful exchanges in domains as
various as the discovery of supernovae, photometric follow-up of variable stars,
meteorology of planets, occultations of stars by asteroids, mutual phenomena of
Jupiter’s satellites, etc. It is worth pointing out, in addition, that nowadays amateurs can access numerous 600 mm-class telescopes or telescopes that are smaller
but highly automatised, which are very efficient for sky survey programmes.
In this context, the observation by amateurs takes a new dimension: from a
simple hobby it becomes useful and contributes to a better knowledge of astronomy. Moreover, with this school, the astrophysics scientific community shows its
willingness to open up and share science with a broad audience. The successive
editions of the schools, in 2003, 2006 and 2009, have all been strikingly successful,
and a forthcoming school is planned in 2012.
The successive chapters of this book will provide, to all those who have a true
passion for astronomy, an idea of the state of the art in the various domains it
tackles: the first chapter exposes the basics of physics of light. The following
two chapters present respectively the spectrographs used in amateur astronomy
and the treatment of the data obtained with these instruments. The following
chapters (4 to 7) show examples of spectroscopic applications to the Sun, Be
stars, planetary nebulae, and comets. This book will thus be useful for all, from
the enlightened amateur to the professional.
DOI: 10.1051/eas/1147000
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