Astronomy & Astrophysics is publishing a special feature this week dedicated to the new results obtained with the solar space observatory Hinode, recognizing the impact of Hinode on various branches of solar physics. 

The solar space observatory Hinode was launched in September 2006 [1], with the name "Hinode" meaning sunrise in Japanese. The Hinode satellite carries a solar optical telescope (SOT), an X-ray telescope (XRT), and an EUV imaging spectrometer (EIS). Hinode investigates both the interior and the atmospheric regions of the Sun. Its primary objectives are to address the origin of the Sun's magnetic field, the driving force behind solar eruptive events, and the nature of the hot corona.

As recognition of the impact of Hinode on various branches of solar physics, Astronomy & Astrophysics is publishing a special feature this week consisting of 18 Letters that present the new results obtained with Hinode. These papers focus on the physics of sunspots, the emergence of magnetic flux on the solar surface, and the dynamics in the solar corona. Figure 1 illustrates these topics.

Fig. 1. The articles published in this special feature address (a) the physics of sunspots (Fig. from Sainz Dalda and Bellot Rubio), (b) the MHD simulations of near-surface dynamo (Fig. from Schüssler and Vögler), and (c) the dynamics of the solar corona (Fig. from Chifor et al.)

A handful of these papers are about sunspots, which are still mysterious in several aspects. They highlight the fine structure of the penumbra, which is the ring of radial structures surrounding the dark core of the spots (see Fig. 2). They present new evidence that the penumbra consists of sea-serpent-like magnetic flux tubes, embedded in a background wrapped around these tubes and connected to magnetic features outside the spot.

Fig. 2. Structure of the sunspots as observed with Hinode (paper by Ichimoto et al.)

Several papers also study the dynamics of the solar corona, focusing on active solar regions and coronal mass ejections (CME, also known as transient events, illustrated on Fig. 3). The new Hinode observations show that the standard scenario describing solar flares do not fit microflares. The high resolution of the soft X-ray telescope on Hinode (see Fig. 4) will help to distinguish between different scenarios.

The papers published this week in A&A – which illustrate only a small part of the science with the new data – show new directions in solar research facilitated by the new solar space telescope Hinode. Through observations of all atmospheric layers of the Sun, from the photosphere and chromosphere into the corona, data from the Hinode observatory provide new insight into the structure and dynamics of the solar atmosphere, an important step toward a better understanding of stellar atmospheres in general.

Fig. 3. Coronal mass ejection (CME, also known as a transient event). An animated version of this observation of a CME by SOHO is available here. © ESA/SOHO

Fig. 4. High-resolution X-ray imaging with XRT of an S-shape sigmoid, often preceding a flaring eruption (paper by McKenzie and Canfield).

---

[1] The project is led by the Japan Aerospace Exploration Agency (JAXA), together with the National Astronomical Observatory of Japan (NAOJ), with contributions from the United States and United Kingdom. The European Space Agency (ESA) is providing ground-station coverage through the Svalbard Satellite Station in Norway.

The Astronomy & Astrophysics special feature (volume 481 n°1 – April I 2008) on the science with Hinode includes 18 articles. They are freely available on the A&A web site.

Table of contents of the A&A special feature (and free access to the PDF files)

---

 

Contact persons:

 

• Science:

Dr. Luis Bellot Rubio
Instituto de Astrofisica de Andalucia (CSIC)
Granada, Spain
Email: lbellot (at) iaa.es
Phone: +34 958 230 508

Dr. Hardi Peter, A&A Editor
Kiepenheuer-Institut fuer Sonnenpysik
Freiburg, Germany
Email: peter (at) kis.uni-freiburg.de
Phone: +49 761 3198 230

• Press office:

Dr. Jennifer Martin
Astronomy & Astrophysics
61, avenue de l'Observatoire
75014 Paris, France
Phone: +33 1 43 29 05 41 - Email: aanda.paris (at) obspm.fr

 

© Astronomy & Astrophysics 2008