(Topic 3. Existing facilities and data bases)

Slides:

Advertisements

Similar presentations

The Sun in all its Glory Here is a look at the sun using many different scanning techniques, as well as different Lenses.

Advertisements

Standard stars for the ZIMPOL polarimeter

Use of the Frequency Agile Solar Radiotelescope for Space Weather A New Solar-dedicated Radio Facility Dale E. Gary, NJIT; Stephen M. White, U Maryland.

Coronal Magnetograph for Space and Ground-based Solar Observatories Silvano Fineschi Alessandro Bemporad, Gerardo Capobianco, Jessica Girella INAF –Astrophysical.

Large amplitude transverse oscillations in a multi-stranded EUV prominence centre for fusion, space and astrophysics J. M. Harris C. Foullon, V. M. Nakariakov,

Space weather at University of Graz / Kanzelhöhe Observatory Institute of Physics, University of Graz, Austria Kanzelhöhe Observatory, Gerlitzen (Austria)

High Altitude Observatory (HAO) – National Center for Atmospheric Research (NCAR) The National Center for Atmospheric Research is operated by the University.

This work was performed under the auspices of the Significant Opportunities in Atmospheric Research and Science Program. SOARS is managed by the University.

Infrastructure and facilities available at INAF – Catania Astrophysical Observatory Salvo Scuderi – INAF OACT 1st SPRING Workshop, Nov 26-28, 2103.

SWD 2005, Taormina, Jun,19-26 An EUV Imaging Detector of Space Solar Telescope Qian Song, Binxun Ye, Zhaowang Zhao National Astronomical Observatories,

Evolution of Barb-Angle and Partial Filament Eruption J.T. Su [1,2], Y. Liu [2], H.Q. Zhang [1], H. Kurokawa [2] V. Yurchyshyn [3] (1)National Astronomical.

The Relation between Filament Skew Angle and Magnetic Helicity of Active Regions Masaoki HAGINO, Y.J. MOON (Korea Astronomy and Space Science Institute)

High Altitude Observatory (HAO) – National Center for Atmospheric Research (NCAR) The National Center for Atmospheric Research is operated by the University.

Characterization of Hα Filbril Structure YUAN Space Weather Research Lab Oct. 26 th, 2010.

SECCHI_CDR_HW_Overview.1 Discussion of Synoptic Program and Use of SSR2 SECCHI Consortium SECCHI Consortium meeting 7 March 2007 Univ. Paris XI.

AGU – Fall 2006 The Solar Polar Field – Cycles 21 – 23 The Solar Polar Field During Solar Cycles J. Todd Hoeksema, Yang Liu, XuePu Zhao & Elena Benevolenskaya.

High-latitude activity and its relationship to the mid-latitude solar activity. Elena E. Benevolenskaya & J. Todd Hoeksema Stanford University Abstract.

Ingolf E. Dammasch ROB/SIDC Brussels, Belgium Solar UV Spectroscopy with SUMER on SOHO (extended version for 11 Oct 2007)

Alfvén Waves in the Solar Corona S. Tomczyk, S. Mclntosh, S. Keil, P. Judge, T. Schad, D. Seeley, J. Edmondson Science, Vol. 317, Sep., 2007.

1Yang LiuCISM All-hand meeting CISM All-hand Meeting Yang Liu – Stanford University

Identifying and Modeling Coronal Holes Observed by SDO/AIA, STEREO /A and B Using HMI Synchronic Frames X. P. Zhao, J. T. Hoeksema, Y. Liu, P. H. Scherrer.

1 A Statistical Study about Transequatorial loops Jie Chen National Astronomical Observatories Chinese Academy of Sciences.

ChroMag 1 Chromospheric Science and ChroMag Alfred de Wijn, Scott McIntosh, Michael Thompson High Altitude Observatory NCAR.

Solar Instruments for Observing the Sun David Groski Mt Cuba Observatory.

Predictions of Solar Wind Speed and IMF Polarity Using Near-Real-Time Solar Magnetic Field Updates C. “Nick” Arge University of Colorado/CIRES & NOAA/SEC.

1 Long-term Solar Synoptic Measurements with Implications for the Solar Cycle Leif Svalgaard Stanford University 23 April 2013.

ISWI in Slovakia ABSTRACT I. DOROTOVIČ ISWI National Coordinator in the Slovak Republic Slovak Central Observatory, Hurbanovo, Slovak Republic,

1 Future solar missions (Based on the summary by R.A. Harrison) S. Kamio

Digitization in Kodaikanal Observatory References and useful links :

P. Gömöry, J. Ambróz, J. Koza, M. Kozák, A. Kučera, J. Rybák, P. Schwartz S. Tomczyk, S. Sewell, P. Aumiller, R. Summers, L. Sutherland, A. Watt Astronomical.

Apodized Filter IWA (λ/D)2~4 OWA (λ/D)13 Contrast ~10 -7 Throughput (%)41.4% Shape of the filter and the simulated coronagraphic point spread function.

Solar local and global magnetism new challenge for long-lasting synoptic observations. (Topic 1. New and continuing scientific questions) A.Kučera, P.

Three Dimensional Visualization of the Solar Corona and study of coronal cavity observed by Yohkoh/SXT and Hinode/XRT J. Okumura, D. Mineyama, H. Watanabe,

Polarized V-band Stars for In-flight Calibration of Space-borne Solar Coronagraphs Capobianco, Gerardo; Fineschi, Silvano INAF- Osservatorio Astrofisico.

Proxies of the Entire Surface Distribution of the Photospheric Magnetic Field Xuepu Zhao NAOC, Oct. 18, 2011.

High Resolution Imaging and EUV spectroscopy for RHESSI Microflares S. Berkebile-Stoiser 1, P. Gömöry 1,2, J. Rybák 2, A.M. Veronig 1, M. Temmer 1, P.

Observational signatures for shocks in the solar photosphere – possible HINODE/SOT observations Jan Rybak and A. Kucera, A. Hanslmeier, H. Woehl Astronomical.

Micro-Flare and High-Speed Down-Flow observed with VTT R. Kano(1), Y. Katsukawa(1), Y. Kitakoshi(2), T. Shimizu(3), S. Tsuneta(1) and V. Martinez Pillet(4)

Near Infrared Spectro-polarimeter (NIRSP) Conceptual Design Don Mickey Jeff Kuhn Haosheng Lin.

Coronal Spectro- polarimetry with the Turin Lyot-Filter Silvano Fineschi INAF – Astrophysical Observatory of Torino, Italy Future of Polarimetry - Brussels.

A.Kučera 1, S. Tomczyk 2, J. Ambróz 1, S. Sewell 2, J. Rybák 1, P. Aumiller 2, P. Gömöry 1, R. Summers 2, P. Habaj 1, L. Sutherland 2, J. Kavka 1, A. Watt.

Observations of Moreton waves with Solar-B NARUKAGE Noriyuki Department of Astronomy, Kyoto Univ / Kwasan and Hida Observatories M2 The 4 th Solar-B Science.

NoRH Observations of Prominence Eruption Masumi Shimojo Nobeyama Solar Radio Observatory NAOJ/NINS 2004/10/28 Nobeyama Symposium SeiSenRyo.

IMF Prediction with Cosmic Rays THE BASIC IDEA: Find signatures in the cosmic ray flux that are predictive of the future behavior of the interplanetary.

N. Petrov, P. Duchlev, K. Koleva, M. Dechev Institute of Astronomy and National Astronomical Observatory ROZHEN, BAS 72 Tsarigradsko Chaussee, Sofia 1784,

OBSERVING THE SUN & PLANETARY TRANSITS Petr HEINZEL Solar Physics Department Astronomical Institute of the Academy of Sciences Czech Republic.

The Sun Youra Taroyan. Age 4.5 ×10 9 years Mean diameter 1.392×10 6 km, 109 × Earth Mass ×10 30 kg, 333,000 × Earth Volume 1.412×10 18 km 3, 1,300,000.

VIIth Bulgarian-Serbian Astronomical Conference, 1- 4 June 2010, Chepelare, Bulgaria The INASAN Zvenigorod observatory plate collection Sergei V. Vereshchagin,

Ganghua Lin Huairou Solar Observating Station,NAO,CAS.

The Mauna Loa Solar Observatory (MLSO) Data Archive Tony Darnell Joan Burkepile and Andrew Stanger High Altitude Observatory P.O.

Sunspot activity and reversal of polar fields in the current cycle 24 A.V. Mordvinov 1, A.A. Pevtsov 2 1 Institute of Solar-Terrestrial Physics of SB RAS,

Three-Dimensional Structure of Coronal Mass Ejections From LASCO Polarization Measurements K. P. Dere, D. Wang and R. Howard ApJL, 620; L119-L

Space Solar Telescope (SST) —— 申请发改委 “ 十二五 ” 项目 Proposed by Chinese Academy of Sciences and China Aerospace Science and Technology Corporation.

Fabry-Perot Approach to SPRING Sanjay Gosain NSO.

The HMI Instrument. HMI Science Goals Line-of-Sight Observables.

Digitization in Kodaikanal Observatory

Good Luck! Final Exam Review Phys 222 – Supplemental Instruction

Cold plasma rotation in the tornado-like prominence of July 13, 2014: a real motion or an illusive effect? J. Rybák1, J. Ambróz1, P. Gömöry1, J. Kavka1,

Hiroko Watanabe (Kyoto Univ.)

Dynamics of the lower solar chromosphere using CRISP-SST data Arnold Hanslmeier(1), Teimuraz Zaqarashvili (1), Julius Koza (2), Jan Rybak (2) (1) Institut.

PSP, SO, and Ground-based Synoptic Observations from NSO

The Sun: Portrait of a G2V star

Detectors of the New Projects at NAOC

The Sun Chapter 17.

Long-Term Variation of Latitudinal Distribution of Coronal Holes

Current Status of ROLO and Future Development

Pavol Rapavý and Daniela Rapavá

Ju Jing, Vasyl B. Yurchyshyn, Guo Yang, Yan Xu, and Haimin Wang

Ron Moore and Alphonse Sterling

Filament/Prominence Eruption Corona Mass Ejection (CME)

Presentation transcript:

(Topic 3. Existing facilities and data bases) Existing solar physics facilities and data bases at the Astronomical Institute of the Slovak Academy of Sciences. (Topic 3. Existing facilities and data bases) A. Kučera, J. Rybák, P. Gömöry, V. Rušin Astronomical Institute, Slovak Academy of Sciences, SK-05690 Tatranská Lomnica, Slovakia ABSTRACT: A brief summary of existing solar physics synoptic facilities and data bases at the Astronomical Institute of the Slovak Academy of Sciences Observations and data sets from the Double coronagraph at Lomnický štit observatory "Homogeneous series of coronal green line intensities"(1939 - present) „Catalogue of solar Hα prominences“ (1967-present) 1st SPRING Workshop, November 26 – 28, 2013, Titisee, Germany 1

Astronomical Institute of the Slovak Academy of Sciences

Astronomical Institute of the Slovak Academy of Sciences

Astronomical Institute of the Slovak Academy of Sciences

CoMP (2012) spectrograph Solar Chromospheric Detector SCD (2014 - 2015) (similar to ChroMag) (P. Gömöry talk)

Topic 3. Existing facilities and data bases Homogeneous series of coronal green line intensities (1939 - present) 1st SPRING Workshop, November 26 – 28, 2013, Titisee, Germany 9

Topic 3. Existing facilities and data bases Homogeneous series of coronal green line intensities (1939 - present) 1st SPRING Workshop, November 26 – 28, 2013, Titisee, Germany 10

Topic 3. Existing facilities and data bases Homogeneous series of coronal green line intensities (1939 - present) 1st SPRING Workshop, November 26 – 28, 2013, Titisee, Germany 11

Topic 3. Existing facilities and data bases Homogeneous series of coronal green line intensities (1939 - present) 1st SPRING Workshop, November 26 – 28, 2013, Titisee, Germany 12

Topic 3. Existing facilities and data bases Homogeneous series of coronal green line intensities (1939 - present) 1st SPRING Workshop, November 26 – 28, 2013, Titisee, Germany 13

rotational characteristics, separately for hemispheres.... Topic 3. Existing facilities and data bases Homogeneous series of coronal green line intensities (1939 - present) Intensity variation, rotational characteristics, separately for hemispheres.... 1st SPRING Workshop, November 26 – 28, 2013, Titisee, Germany 14

Topic 3. Existing facilities and data bases Homogeneous series of coronal green line intensities (1939 - present) green line intensities Blue and yellow mark magnetic field of opposite polarity 1st SPRING Workshop, November 26 – 28, 2013, Titisee, Germany 15

Topic 3. Existing facilities and data bases Catalogue of solar Hα prominences (1967-present) Long-term catalogue of positions, areas, brightness of the H alpha prominences derived from the coronagraphic observations: coronagraph ZEISS 200/3000, interference filter - ~0.6 nm, film,... Papers “Catalogue of solar prominences (1967 – 1986)”, Rušin, V.; Rybanský, M.; Dermendjiev, V.; Stavrev,. Ya., CAOSP, Vol. 17, p. 63 – 292, 1988 “Catalogue of solar prominences 1987 – 1993”, Rusin, V.; Rybansky, M.; Dermendjiev, V.; Stavrev, K. Ya., CAOSP Supplement, vol. 24, p. 135-136, 1994 16

photographic film, 36x24mm, several exposures along the limb Topic 3. Existing facilities and data bases Catalogue of solar Hα prominences (1967-present) photographic film, 36x24mm, several exposures along the limb development with a high contrast, projection for a large image drawing of shapes of prominences, measurement of the parameters: position angle, limb, latitude, longitude, area, height, subjective brightness (1-2-3) observations: coronagraph ZEISS 200/3000, interference filter - ~0.6 nm, film,... 17

Free post-focal space needed for new instruments – CoMP-S, SECIS,... Topic 3. Existing facilities and data bases Catalogue of solar Hα prominences (1967-present) Because of: Free post-focal space needed for new instruments – CoMP-S, SECIS,... End of the coronagraphic photographic observations at the LSO – 20/09/2009 we asked for introduction of the full-disk H alpha observations with an extended exposure time for prominences at the Kaznelhőhe Solar Observatory KSO Starting from 8/2009 18

KSO LSO Topic 3. Existing facilities and data bases Catalogue of solar Hα prominences (1967-present) KSO LSO 19

oo Topic 3. Existing facilities and data bases Catalogue of solar Hα prominences (1967-present) oo 1st SPRING Workshop, November 26 – 28, 2013, Titisee, Germany 20

Topic 3. Existing facilities and data bases Catalogue of solar Hα prominences (1967-present) 1st SPRING Workshop, November 26 – 28, 2013, Titisee, Germany 21

Topic 3. Existing facilities and data bases Catalogue of solar Hα prominences (1967-present) 1st SPRING Workshop, November 26 – 28, 2013, Titisee, Germany 22

Topic 3. Existing facilities and data bases Catalogue of solar Hα prominences (1967-present) Prominences distribution Blue and yellow mark magnetic field of opposite polarity 1st SPRING Workshop, November 26 – 28, 2013, Titisee, Germany 23

Thank you 24