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WP1: Solar activity and its influence on the heliosphere and geospace
WP2: Influence of solar variability on Earth's climate
WP3: Eruptive activity of late-type and sun-like stars
WP4: Radiative processes in solar and stellar atmospheres
WP5: Search for exoplanets and/or sub-stellar companions
WP6: Dissemination, teaching and public outreach
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Milestones
- R. Brajša
- H. Božić
- J. Čalogović
- M. Dumbović
- R. Jurdana-Šepić
- I. Poljančić-Beljan
- D. Ruždjak
- D. Sudar
- B. Vršnak
- T. Žic
Milestones details
31. October 2014
M01 - Completing the coronagraphic and EUV data sets
M02 - Completing coronal shock formation modelling
M03 - Analysis of solar activity strength by precursor and extrapolation methods
30. November 2014
M04 - Finalizing IDL programmes for calculating intensity and brightness temperature as a function of wavelength, using different models of the solar atmosphere
M05 - Obtain a catalogue of all short-events with largest deviations in CR flux (Forbush decreases & GLE events)
M06 - Calculation of meridional and rotation velocities, Reynolds stresses and development of a random walk model based on coronal bright points from SDO
M07 - Set of methods capable to reliably test the statistical significance of the results obtained using the geophysical data
M08 - Sample of program stars and observation plan
M09 - Completing test observations
M10 - BVR magnitudes of selected objects
31. December 2014
M11 - Completing the in situ ICME data sets
M12 - Completing modelling of coronal shock propagation
28. February 2015
M13 - Finalizing compilation of data sets
M14 - Determination of quality and the best processing methods for the satellite cloud data
M15 - Completing solar activity observations
M16 - Finalizing the observing campaign programme
M17 - Expanding of existing UBVR archives
M18 - Completing the geomagnetic data sets
M19 - Completing analysis of shock coronal and chromospheric effects
30. April 2015
M20 - Completing the ICME-related cosmic-ray data
M21 - Completing observational data set
31. May 2015
M22 - Completing the analysis and interpretation
M23 - Potential limits of cloud datasets to detect a small changes in clouds related to solar activity are known
M24 - Completing the program stars dataset
M25 - Increase of the light gathering power on 1-m telescope
M26 - UBVR magnitudes of selected stars
30. June 2015
M27 - Completing the CIR-related EUV coronal hole and in situ data sets
M28 - Completing analysis of observational data
31. August 2015
M29 - Better understanding of cosmic ray-cloud hypothesis
M30 - Application of developed methods to various geophysical data
M31 - Completing the analysis of the eruptive activity of young pre-main sequence objects
M31 - UBVR magnitudes of selected stars
M33 - Completing solar activity observations
M33 - Completing test observations
M34 - BVR magnitudes of selected objects
M35 - Completing the CIR-related geomagnetic and cosmic-ray data
M36 - Completing analysis of modelling and observational results and their comparison
M37 - Data compilation finished
M38 - Completing coronal shock study
30. November 2015
M40 - Completing the interpretation of the relationship between remote and in situ observations of solar eruptions; implications for space weather effects
M41 - Finalizing compilation of data sets
29. February 2016
M42 - Completing the interpretation of the geoeffectiveness of solar eruptive events
M43 - Calculation of meridional and rotation velocities and Reynolds stresses based on sunspot data from Kanzelhohe and Debrecen
M44 - Completing the analysis and interpretation
31. May 2016
M45 - Completing the interpretation of the relationship between coronal hole observations and in situ CIR measurements
M46 - Preliminary modelling
M47 - Finalizing compilation of data sets
31. August 2016
M48 - Completing the interpretation of the geoeffectiveness of solar eruptive events
M49 - Preliminary modelling the effects of reconnection
M50 - Completing solar activity observations
M51 - Analysis of solar rotation and activity
M52 - UBVR magnitudes of selected stars
M53 - Completing the analysis and interpretation
M54 - Data analysis and interpretation finished
31. October 2016
M55 - Validation of the real-time forecasting and finishing public online CME-arrival forecasting tool
30. November 2016
M56 - Finalizing compilation of data sets
31. December 2016
M57 - Validation of the real-time forecasting and finishing public online CIR-onset forecasting tool
28. February 2017
M58 - Completing the analysis and interpretation
M59 - BVR magnitudes of selected objects
M60 - Validation of the real-time forecasting and finishing public online CME-forecasting tool
31. May 2017
M61 - Validation of the real-time forecasting and finishing public online CME/CIR space weather forecasting tool
M62 - Completing solar activity observations
M63 - Better understanding of centennial climate variations related to bottom up mechanism
31. August 2017
M64 - Better determination of local and regional solar influences on clouds
M65 - 1st-step evaluation of the real-time space weather forecasting and finishing public online CME/CIR space weather forecasting tool
M66 - Finalizing modelling
M67 - Research on the geoeffectiveness of solar eruptive events and corotating interaction regions finished
30. November 2017
M68 - Completing solar activity observations
M69 - Better understanding of theoretical changes in cloud properties related to the global electric circuit
M70 - UBVR magnitudes of selected stars
M71 - BVR magnitudes of selected objects
31. December 2017
M72 - Adjustment of the real-time space weather forecasting tool and completing public online CME/CIR space weather forecasting tool
M73 - Completing solar activity observations
28. February 2018
M74 - Investigation of centennial climate variations related to changes in solar activity
31. May 2018
M75 - Synthesis of the most important conclusions
M76 - Archive of UBVR magnitudes and light curves of selected T-Tauri stars
30. June 2018
M77 - Final evaluation of the real-time space weather forecasting and finishing public online CME/CIR space weather forecasting tool
31. August 2018
M78 - Determination of most favorable mechanisms explaining influence of solar activity on climate
M79 - Finalizing BVR photometric observations