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Sanchita Pal
Centre of Excellence in Space Sciences, India Indian Institute of Science Education and Research Kolkata Mohanpur-741246 West Bengal Citizenship: Indian Gender: Female Sanchita Pal Field of research: The solar origin of space weather and its terrestrial impact and an overall assessment of the pathways through which space weather impacts are mediated and thus to predict the space weather disturbances. Name of institute: Center of Excellence in Space Sciences, India, IISER Kolkata. Pursuing degree: Ph.D. Completed degree (in descending order): M.Tech in Radio Physics and Electronics (Specialization: Space science). B.Tech in Electronics and Communication Engineering. Poster presentations : Poster on ‘Investigating the cause of fewer geomagnetic storm during the higher peak of the double-peaked sunspot cycle 24’ in the international conference, ‘Science for Space weather’, held on January,2016,Goa,India. Schools/Workshops Attended (in descending order): CCMC Space weather Concepts and Tools. (2016). IRIS-5 workshop held on Inter- University Institute of Astronomy and Astrophysics (IUCAA), Pune. IMPRESS-2015 (Inspiring the Minds of Post-graduates for Research in Earth and Space Sciences - 2015) organized by Indian Institute of Page 1 of 4 Geomagnetism (IIG), Navi Mumbai at Equatorial Geomagnetic Research Laboratory (EGRL), Tirunelveli. Purpose of study in the research field : Space weather impact is one of the serious issues in recent world. Many significant models, systems have been generated to observe and analysis space weather in broad way. Now the most important thing is to predict the space weather some time before so that measurements can be taken for the hazards. My purpose of study is to contribute in predicting the space weather impacts by observing their sources on solar surface with the help of some predefined models. -
We Have Our Own MSSQL Database That Gathers All the Information
International Astronomical Union Union Astronomique Internationale POST MEETING REPORT FORM Deadline for Submission: within 1 month after the meeting For Symposia the following documents should be attached: (i) Final scientific program, list of invited review speakers and session chairs; (ii) Summary of the scientific highlights of the meeting (1 page, to be published on the IAU website); (iii) List of participants, including their distribution by country and gender (double bar chart); (iv) List of recipients of IAU grants, stating the amount received, country and gender; (v) An Executive Summary of the Meeting (1-2 pages) to be published on the IAU website. For Symposia the Post Meeting Report should be sent to the AGS. For Focus Meetings the Post Meeting Report should include the documents referred to above in (i), (ii) and (v) and be sent to the GS. For Regional Meetings the Post Meeting Report should include the documents referred above fromm (i) to (v), as well as a proposal for the next venue, and be sent to the GS. 1. Meeting Number: 2. Meeting Title: 3. Coordinating Division: 4. Dedication of meeting (if any): 5. Location (city, country): 6. Dates of meeting: 7. Number of participants: 8. List of represented countries: 9. Report submitted by: 10. Date and place: 11. Signature of SOC Chairperson: POST MEETING REPORT IAU Symposium 335 Space Weather of the Heliosphere: Processes and Forecasts Symposium photograph taken on 19th July 2017. Table of Contents (i) Final scientific program 2 List of invited review speakers and session chairs 2 Oral Program 3 Poster Program 12 (ii) Summary of the scientific highlights 18 (iii) List of participants 19 (iv) List of recipients of IAU grants 25 (v) Executive Summary 26 1 (i) Final scientific program, list of invited review speakers and session chairs We list invited speakers and session chairs below and the next pages detail the scientific oral and poster programs, with any corrections from the published conference booklet. -
Nandi Dibyendu Indo
Indo-US Bilateral Cooperation Program in Heliophysics and Space Weather Dibyendu Nandy ~~ Indian Institute of Science Education and Research, Kolkata What is Heliophysics? • Solar variability forces space environment and planetary atmospheres • Characterize space weather and climate • System-wide studies defines the science of Heliophysics http://en.wikipedia.org/wiki/Heliophysics http://science.nasa.gov/heliophysics/ Why heliophysics? Sun Creates Space Weather Hinode • Sunspots are strongly magnetized regions • Solar storms originate within sunspots and travel to Earth in few days • Solar flares and coronal mass ejections (CMEs) – biggest explosions in the solar system – eject magnetized plasma and charged particles (m ~ 10 12 Kg, v ~ 500-2000 km/s, E ~ 10 24 Joules, 10 12 atom bombs) Space Weather Effects: Satellite Operations, Telecommunications • Satellite operations (charging: interferes with electronic circuitry) • Space walks (exposes astronauts to high radiation) • Disrupts telecommunication systems (GPS, Satellite TV broadcasts) Space Weather: Radio Communications & Flights HF Communication only • Solar plasma and magnetic fields get through the Earth’s polar (open magnetic field) regions; auroras are caused by geomagnetic stomrs • Affects air-traffic over polar routes Space Weather Effects: Geomagnetic Storms, Electric Facilities • Effect of solar storms felt at ground level at high latitudes • Induces large voltages in northern oil pipelines, fire hazards • Trips electric power grids Space Weather Affects Critical Technologies -
Effects of the Solar Cycles and Longer-Term
University of New Hampshire University of New Hampshire Scholars' Repository Doctoral Dissertations Student Scholarship Summer 2019 Effects of the Solar Cycles and Longer-Term Solar Variations: Modulation of Galactic Cosmic Radiation and Filtration of Neutral Atoms from the Local Interstellar Medium Fatemeh Rahmanifard University of New Hampshire, Durham Follow this and additional works at: https://scholars.unh.edu/dissertation Recommended Citation Rahmanifard, Fatemeh, "Effects of the Solar Cycles and Longer-Term Solar Variations: Modulation of Galactic Cosmic Radiation and Filtration of Neutral Atoms from the Local Interstellar Medium" (2019). Doctoral Dissertations. 2483. https://scholars.unh.edu/dissertation/2483 This Dissertation is brought to you for free and open access by the Student Scholarship at University of New Hampshire Scholars' Repository. It has been accepted for inclusion in Doctoral Dissertations by an authorized administrator of University of New Hampshire Scholars' Repository. For more information, please contact [email protected]. Effects of the Solar Cycles and Longer-Term Solar Variations: Modulation of Galactic Cosmic Radiation and Filtration of Neutral Atoms from the Local Interstellar Medium BY Fatemeh Rahmanifard B.Sc., Amirkabir University of Technology, 2007 M.Sc., Amirkabir University of Technology, 2011 THESIS Submitted to the University of New Hampshire in Partial Fulfillment of the Requirements for the Degree of Doctor of Philosophy in Physics September, 2019 ALL RIGHTS RESERVED c Year My Name ii This thesis has been examined and approved in partial fulfillment of the requirements for the degree of Doctor of Philosophy in Physics by: Thesis Director, Dr. Nathan Schwadron, Presidential Chair, Norman S. and Anna Marie Waite Physics Professor Dr. -
Exploring the Origin and Dynamics of Solar Magnetic Fields
EXPLORING THE ORIGIN AND DYNAMICS OF SOLAR MAGNETIC FIELDS Soumitra Hazra Department of Physical Sciences and Centre of Excellence in Space Sciences India Indian Institute of Science Education and Research Kolkata arXiv:1604.00563v1 [astro-ph.SR] 2 Apr 2016 This dissertation is submitted for the degree of Doctor of Philosophy in Science 2015 Dedicated to My Parents... Declaration This thesis is a presentation of my original research work. Wherever contributions of others are involved, every effort is made to indicate this clearly, with due reference to the literature and acknowledgments of collaborative research and discussions. The work has not been submitted earlier either in entirety or in parts for a degree or diploma at this or any other Institution or University. Some chapters of this thesis have either been published or are in the process of being published. This work was done under the guidance of Dr. Dibyendu Nandi, at the Indian Institute of Science Education and Research Kolkata (IISER Kolkata). Soumitra Hazra 2015 CERTIFICATE FROM THE SUPERVISOR This is to certify that this thesis entitled "Exploring the Origin and Dynamics of Solar Magnetic Fields" – which is being submitted by Soumitra Hazra (who registered on 11th August, 2009 for a PhD Degree with registration number 09RS028 at the Indian Institute of Science Education and Research Kolkata) – is based upon his own research work under my supervision and that neither this thesis nor any part of it has been submitted for any degree or any other academic award anywhere else. Dr. Dibyendu Nandi Associate Professor Department of Physical Sciences and Center of Excellence in Space Sciences India Indian Institute of Science Education and Research Kolkata West Bengal 741246 India Acknowledgements This is a special moment for me and I wish to express my sincere gratitude to my thesis supervisor Dibyendu Nandi, who introduced me to the exciting world of research in Astro- physics. -
DIBYENDU NANDI Assistant Professor, Physics Indian Institute of Science Education and Research, Kolkata Mohanpur -741252, West Bengal [email protected]
RAMANUJAN FELLOWS DIBYENDU NANDI Assistant Professor, Physics Indian Institute of Science Education and Research, Kolkata Mohanpur -741252, West Bengal [email protected] Dibyendu Nandi obtained his B.Sc. degree (1995) from St. Xavier's College, Calcutta University and his M.S. and Ph.D. degrees (2002) in Physics from the Indian Institute of Science, Bangalore. He did postdoctoral work at Montana State University and subsequently held positions of Research Scientist and Assistant Professor there. Dibyendu returned to India in 2008 and joined IISER Kolkata. He continues to hold Visiting positions at Montana State University and Harvard-Smithsonian Center for Astrophysics. RESEARCH DESCRIPTION Dibyendu Nandi's research is directed towards understanding the origin of the Sun's magnetic activity and its impact on our space environment, climate and modern-day technologies. The activity of the Sun is governed by its variable magnetism which is produced by a magnetohydrodynamic dynamo mechanism in the solar interior. Solar magnetic fields spawn flares and coronal mass ejections which are the largest explosions in the solar system. These solar storms impact satellite operations, telecommunications, air-traffic over polar routes, electric grids and oil pipelines in high-latitude countries. The long-term variation of solar magnetic fields also modulates the Sun's energy output and is therefore relevant for the the climate system. Dibyendu's research has contributed to the understanding of how plasma flows inside the Sun influence magnetic field generation. In particular, using computational models, he has made important contributions to understanding the role of a large-scale flow of plasma known as meridional circulation in the spatio-temporal evolution of sunspots - strongly magnetized structures in the Sun which were first systematically observed by Galileo Galilei. -
Acknowledgement to Reviewers
381 Acknowledgement to Reviewers The Publisher and the Editor of Indian Journal of Radio & Space Physics gratefully acknowledge the honorary services rendered by the following experts in reviewing the papers during 2010: Dr M A Abdu Dr O P N Calla Inst Nacl Pesquisas Espaciais International Centre for Radio Science BR-12201 Sao Jose Dos Campos, Brazil A-23, Shastri Nagar, Jodhpur 342 003, Rajasthan [email protected], [email protected] Prof S K Chakrabarti Prof S P Agrawal Department of Astrophysics & Cosmology Asha Kiran Building, Sirmour Chauraha S N Bose National Centre for Basic Sciences Civil Lines, Rewa (MP) 486 001 Sector-III, Block JD, Salt Lake, Kolkata - 700 098 [email protected] Prof H S Ahluwalia Prof D K Chakrabarty Dept of Physics and Astronomy Centre for Environment Survey The University of New Mexico, New Mexico 87131-0001 Vidyanagar Society 29/251, Ahmedabad 380 015 [email protected] [email protected] Dr (Mrs) R C Aiyer Dr D Chand Department of Physics, Pune University, Pune 411 008 Dept Atmospher Sci, Univ Washington, Seattle, WA 98195 USA [email protected] [email protected], [email protected] Dr K V S Badarinath Prof Arnab Rai Choudhuri Atmospheric Science Section, National Remote Sensing Centre Department of Physics ISRO, Dept of Space, Balanagar, Hyderabad 500 625 (AP), India Indian Institute of Science, Bangalore 560 012, Karnataka India [email protected] [email protected] Dr Badruddin Prof S S De Department of Physics Dept of Radiophysics & Electronics, S K Mitra -
On the Current Solar Magnetic Activity in the Light of Its Behaviour During the Holocene
On the current solar magnetic activity in the light of its behaviour during the Holocene F. Inceoglu Stellar Astrophysics Centre, Department of Physics and Astronomy, Aarhus University, Ny Munkegade 120, DK-8000 Aarhus C, Denmark Department of Geoscience, Aarhus University, Høegh-Guldbergs Gade 2, DK-8000 Aarhus C, Denmark [email protected] R. Simoniello Laboratoire AIM, CEA/DSM-CNRS-Universit´eParis Diderot, IRFU/SAp, Centre de Saclay, F-91191, Gif-sur-Yvette, France [email protected] M. F. Knudsen Department of Geoscience, Aarhus University, Høegh-Guldbergs Gade 2, DK-8000 Aarhus C, Denmark C. Karoff Stellar Astrophysics Centre, Department of Physics and Astronomy, Aarhus University, Ny Munkegade 120, DK-8000 Aarhus C, Denmark Department of Geoscience, Aarhus University, Høegh-Guldbergs Gade 2, DK-8000 Aarhus C, Denmark J. Olsen AMS, 14C Dating Centre, Department of Physics, Aarhus University, Ny Munkegade 120, DK-8000 Aarhus C, Denmark arXiv:1509.06182v1 [astro-ph.SR] 21 Sep 2015 S. Turck-Chi`eze Laboratoire AIM, CEA/DSM-CNRS-Universit´eParis Diderot, IRFU/SAp, Centre de Saclay, F-91191, Gif-sur-Yvette, France ABSTRACT Solar modulation potential (SMP) reconstructions based on cosmogenic nuclide records reflect changes in the open solar magnetic field and can therefore help us obtain { 2 { information on the behaviour of the open solar magnetic field over the Holocene period. We aim at comparing the Sun's large-scale magnetic field behaviour over the last three solar cycles with variations in the SMP reconstruction through the Holocene epoch. To achieve these objectives, we use the IntCal13 14C data to investigate distinct patterns in the occurrences of grand minima and maxima during the Holocene period. -
Arxiv:1802.05628V1 [Astro-Ph.SR] 15 Feb 2018 Sunspot Number of R = 116 (Revised Value ) Or R = 70 (Unrevised Value), About
Precursors of an upcoming solar cycle at high latitudes from coronal green line data K. Petrovay, M. Nagy, T. Gerj´ak E¨otv¨osUniversity,Department of Astronomy, Budapest, Hungary L. Juh´asz E¨otv¨osUniversity,Department of Geophysics and Space Science, Budapest, Hungary Abstract After reviewing potential early indicators of an upcoming solar cycle at high latitudes, we focus attention on the rush{to-the-poles (RTTP) phenomenon in coronal green line emission. Considering various correlations between properties of the RTTP with the upcoming solar cycle we find a correlation between the rate of the RTTP and the time delay until the maximum of the next solar cycle. On the basis of this correlation and the known internal regularities of the sunspot number series we predict that, following a minimum in 2019, cycle 25 will peak in late 2024 at an amplitude of about 130 (in terms of smoothed monthly revised sunspot numbers). This slightly exceeds the amplitude of cycle 24 but it would still make cycle 25 a fairly weak cycle. Keywords: Sun, solar activity, solar cycle, sunspot number 1. Introduction Solar Cycle 25 reached its maximum in April 2014 with a 13-month smoothed 1 arXiv:1802.05628v1 [astro-ph.SR] 15 Feb 2018 sunspot number of R = 116 (revised value ) or R = 70 (unrevised value), about ∗Corresponding author Email address: [email protected] (K. Petrovay) 1The revision of the official sunspot number series that took place in 2015 was a well known crucial milestone in recent solar physics. For more explanations see http://sidc.oma.be/silso/newdataset Preprint submitted to Journal of LATEX Templates February 16, 2018 30 % lower than an average cycle and roughly half the typical amplitude of cycles 18{23, comprising the Modern Maximum. -
Arxiv:1907.02107V2 [Astro-Ph.SR] 4 Mar 2020 E-Mail: [email protected] 2 Krist´Ofpetrovay
Living Reviews in Solar Physics manuscript No. (will be inserted by the editor) Solar cycle prediction Krist´ofPetrovay Received: date / Accepted: date Abstract A review of solar cycle prediction methods and their performance is given, including early forecasts for Cycle 25. The review focuses on those aspects of the solar cycle prediction problem that have a bearing on dynamo theory. The scope of the review is further restricted to the issue of predicting the amplitude (and optionally the epoch) of an upcoming solar maximum no later than right after the start of the given cycle. Prediction methods form three main groups. Precursor methods rely on the value of some measure of solar activity or magnetism at a specified time to predict the amplitude of the following solar maximum. The choice of a good precursor often implies considerable physical insight: indeed, it has be- come increasingly clear that the transition from purely empirical precursors to model-based methods is continuous. Model-based approaches can be further divided into two groups: predictions based on surface flux transport models and on consistent dynamo models. The implicit assumption of precursor methods is that each numbered solar cycle is a consistent unit in itself, while solar activity seems to consist of a series of much less tightly intercorrelated individual cycles. Extrapolation methods, in contrast, are based on the premise that the physical process giving rise to the sunspot number record is statistically homogeneous, i.e., the mathematical regularities underlying its variations are the same at any point of time, and therefore it lends itself to analysis and forecasting by time series methods. -
My Life and My Journey Through Solar Physics
1 My Life and My Journey through Solar Physics Arnab Rai Choudhuri [On 18 February 2018 – one day before the conference International Astronomical Union Symposium 340: Long-Term Datasets for the Understanding of Solar and Stellar Magnetic Cycles (19 – 24 February 2018) – a one-day workshop on Solar-Stellar Magnetism: Past, Present and Future was organized at the same venue (B.M. Birla Auditorium, Jaipur, India). According to the official website of this workshop: This one day workshop is being organized in India on the occasion of Arnab Rai Choudhuri's 60th year to discuss outstanding challenges and future prospects in our understanding of the origin of solar-stellar magnetism – a topic in which Choudhuri has made significant contributions. The scientific sessions will be structured around invited discourses and a panel discussion. The workshop will precede (by one day) the International Astronomical Union Symposium 340 (Long-Term Datasets for the Understanding of Solar and Stellar Magnetic Cycles) and will be held in the same venue. The Organizing Committee consisted of Dibyendu Nandi, IISER Kolkata (SOC Chair); Dipankar Banerjee, IIA; Ramit Bhattacharyya, PRL; Piyali Chatterjee, IIA; Prateek Sharma, IISc; Prasad Subramanian, IISER Pune; Durgesh Tripathi, IUCAA. I was asked to give a 45-minute talk on My Life and My Journey through Solar Physics. Since I have never given such a talk and I was somewhat nervous about it, I wrote down the talk while preparing it – something which I normally would not do for an astrophysics talk. What follows is a polished version of the write-up.] 2 The programme of the workshop. -
Post Meeting Report IAU SYMPOSIUM 340 Long Term Datasets for the Understanding of Solar and Stellar Magnetic Cycles
Post Meeting Report IAU SYMPOSIUM 340 Long Term Datasets for the Understanding of Solar and Stellar Magnetic Cycles Symposium photograph taken on 20th February 2017 Table of Contents 1) Final scientific program 1 a)List of invited review speakers and session chairs 10 b)Oral Program 18 c)Poster Program 22 2) Summary of the scientific highlights 24 3) List of Participants 25 4) List of recipients of IAU grants 26 5) Executive Summary 27 1 (i) Final scientific program, list of invited review speakers and session chairs Following is the list of invited speakers and session chairs and in next pages contain scientific oral and poster programs, with any corrections from the published conference booklet. Invited Speakers (in the order of the Scientific Program) Aaron C Birch (Max Planck Institute for Solar System Research, Germany) Shravan Hanasoge (Tata Institute of Fundamental Research, India) Robert Cameron (Max Planck Institute for Solar System Research, Germany) Sarbani Basu (Yale University, USA) Aimee Norton (Stanford University, USA) Frederic Clette (Royal Observatory of Belgium, Belgium) Andres Munoz-Jaramillo (SouthWest Research Institute, USA) M J Owens (University of Reading, UK) Ilaria Ermolli (INAF Osservatorio Astronomico di Roma, Italy) Nat Gopalswamy (NASA Goddard Space Flight Center, USA) Qi Hao (School of Astronomy and Space Science, Nanjing University, China) Martin Snow (University of Colorado / LASP, USA) Natalie Krivova (Max Planck Institute for Solar System Research, Germany) Travis Metcalfe (Space Science Institute,