FP6Реинтеграция2007–2008

SOND · Solar network dynamics

6РП — Действия „Мария Кюри“

Период
2007-07-01 → 2008-06-30
Финансиране от ЕС
35 600 €
Участници
1
Схема
ERG

Линиите свързват координатора с партньорите. За проекти отпреди 2014 г. CORDIS не винаги дава точни координати. Тези точки са на ниво град или държава.

Накратко на български

Слънчевата хромосфера и преходният регион се анализират чрез наблюдение на динамични фибрили – светли струи от плазма. Това помага да се разбере как се движи енергията и как функционират малките структури в атмосферата на Слънцето.

Този кратък обзор е генериран от изкуствен интелект

Кратко обяснение, генерирано от езиков модел по текста на CORDIS. Оригиналът е по-долу.

Резултати накратко

Final Activity Report Summary - SOND (Solar Network Dynamics)

The project focused on the coupling between network dynamics and fine structures seen in the solar chromosphere and transition region. The scientific objectives involved: (a) small-scale network dynamics, (b) leakage of photospheric oscillations to the chromosphere, and (c) nature of spicules. The project realisation embraced organisation of joint observing campaigns aimed at acquisition of multispectral time sequences with long duration, their later analysis, interpretation, and confrontation with numerical simulations. The project realisation benefited from availability of unprecedented high-resolution image sequence, though brief, obtained in 2002 by the rocket-borne Very high Angular resolution ULtraviolet Telescope (VAULT). The researcher took part actively as a co-proposer and an observer in setup and execution of two joint observing programs with the titles: Dynamic fibrils in the upper photosphere, chromosphere, and above; and Spectroscopy of the quiet solar photosphere: properties of the shocks and the acoustic flux generation. The programs were accomplished successfully by the Vacuum Tower Telescope at Observatorio del Teide, Canary Islands, Spain in May and June 2008. Before the observing campaigns the researcher analyzed VAULT filtergrams in the Ly alpha spectral line searching for dynamic fibrils (DFs) - bright jet-like features emanating from network boundaries and displaying conspicuous extension and/or retraction on timescales of several seconds. The researcher developed a software for measuring of precise image coordinates facilitating first ever identification of DFs in Ly alpha. The project brought the following results towards the objectives (a) and (b): The observing campaigns provided extensive multispectral and spectropolarimetric data volumes sampling the solar atmosphere in infrared and visual spectral ranges from lower photosphere up to the upper chromosphere. Thorough interpretation is a formidable challenge extending beyond project duration. Nevertheless, samples of observations were already presented as image of the month July 2008 at the webpage of Kiepenheuer-Institut fur Sonnenphysik in Freiburg (KIS). They will be presented as a poster in 12th European Solar Physics Meeting (ESPM-12) in September 2008. The project brought the following new results towards the objective (c): 1) most tops of DFs move supersonically; 2) decelerations of DFs vary from sub- to superballistic; 3) about half of DFs show outward acceleration, which may be an artefact from the poor sampling. The similarity between these DFs observed in Ly alpha and the ones observed in Halpha suggests that the magnetoacoustic shock excitation proposed for the Halpha DFs is also valid for the Ly alpha ones. This supports an idea that Halpha and Ly alpha DFs are on-disk manifestation of limb spicules. The most important scientific achievement made by the project so far is the first ever identification of DFs in Ly alpha. This achievement was already presented at several scientific gatherings, submitted as a regular paper in Astronomy and Astrophysics and will be presented as a talk in ESPM-12. The project outcomes are detailed in a publication accessed at URL http://adsabs.harvard.edu/default_service.html by simply entering the researcher's name. The project implementation also involved effective reintegration of the researcher after initial two-years MC Intra-European Fellowship back into his home country Slovakia via permanent employment at the Astronomical Institute, Slovak Academy of Sciences in Tatranska Lomnica (AISAS) located in Vychodne Slovensko (East Slovakia) and classified as less-favoured region of the Community. Simultaneously, the researcher maintained strong linkage and transfer of knowledge between AISAS and leading European institutions through research travels and stays thus enhancing the visibility of his research and home institute in European research area.

Текст от CORDIS, на английски · Данни: CORDIS, © Европейски съюз

Цел на проекта

Our SoND proposal targets multi-wavelength solar atmosphere physics with Canary Islands solar telescopes and space missions. This advanced technology rendering high-resolution tomography, spectroscopy and polarimetry will be involved in exploration of small-scale dynamics in magnetic network and its manifestations in fine chromospheric structures. In this project the applicant's experiences in large-volume inversion will be combined with extensive observational and interpretational expertise of the host institution in quest for:- Small-scale network dynamics;- Leakage of photospheric oscillations to the chromosphere;- Nature of the spicules.The research topic addresses the magnetic interconnection between the photosphere and the outer solar atmosphere, which is far from being understood but arguably influencing the near-Earth environment. The applicant will so continue in research of direct human importance using the modern European solar telescopes and keeping strong linkage to leading re search groups after return to his Slovakian scientific community as a permanent staff member.

Оригинален текст от CORDIS (на английски).

Участници

  • ASTRONOMICKÝ ÚSTAV SLOVENSKEJ AKADÉMIE VIED · VYSOKÉ TATRYКоординаторНиво градСловакия

Връзки

Данни: CORDIS, © Европейски съюз