Geomagnetic Storm measured in Birr on 2nd October 2013. Thought to have been caused by the Coronal Mass Ejection released from the Sun on 29th September
Ultra-fast Outflows from Active Galactic Nuclei of Seyfert I GalaxiesAshkbiz Danehkar
High Energy Phenomena Seminar, Harvard CfA, Cambridge, USA, September 7, 2016, https://doi.org/10.6084/m9.figshare.13699048 https://youtu.be/7q_wv61ou1E
Ultra-fast Outflows from Active Galactic Nuclei of Seyfert I GalaxiesAshkbiz Danehkar
High Energy Phenomena Seminar, Harvard CfA, Cambridge, USA, September 7, 2016, https://doi.org/10.6084/m9.figshare.13699048 https://youtu.be/7q_wv61ou1E
The x ray_outburst_of_the_galactic_centre_magnetar_sgr_j1745_2900_during_the_...Sérgio Sacani
Artigo descreve a pesquisa feita com a magnetar localizada próxima do buraco negro supermassivo da Via Láctea e que tenta explicar o comportamento estranho e incomum desse objeto misterioso.
C5.03: Ocean observations by the Global Change Observation Mission (GCOM) - K...Blue Planet Symposium
As a contribution to the climate variability monitoring, the Japan Aerospace Exploration Agency (JAXA) initiated the Global Change Observation Mission (GCOM). GCOM is a concept comprised of two polar-orbiting satellite series, spread over three generations to achieve long-term and consistent data records. The two satellite series are GCOM-W (Water) and GCOM-C (Climate). JAXA is implementing the first generation of the series. The GCOM-W satellite was launched on May 18, 2012 (Japan Standard Time) and started the continuous observation by the Advanced Microwave Scanning Radiometer-2 (AMSR2) from the A-Train orbit. The instrument has been showing stable performance and accumulating its data records. AMSR2 is capable of observing various oceanic and atmospheric geophysical parameters, including sea surface temperature (SST), sea surface wind speed, water vapor, cloud liquid water, precipitation, and sea ice. Particularly, nearly all-weather SST measurement by utilizing the characteristics of microwave observation is playing an important role in capturing dynamic changes of ocean phenomena, together with the time-proven infrared observations. The GCOM-C satellite is now under development and scheduled for launch in Japanese fiscal year 2016 to provide the continuous observations related to carbon cycle and radiation budget. The satellite will be equipped with the Second-generation Global Imager (SGLI) with some unique features including enhanced spatial resolution (250 m) for most of the visible channels, ultraviolet channels (380 nm), and polarization/multidirectional measurement capabilities. These features will provide the better understanding of the coastal phenomena through the detailed and accurate observations of coastal ocean colors and SST.
GW170817: Dawn of multi-messenger astronomy Amruta Jaodand
A bystander's view of how the detection of first neutron star merger seen by LIGO Scientific Collaboration and Virgo was followed up by electromagnetic observations. Timeline curated from discovery papers, twitter threads and GCN's
Evidence for Long-Lasting Electrical Leader Discharges in NonSpecular Meteor ...researchinventy
Unusual, non-specular, fast-movingmeteortrail echoes are observed in the summer polar upper mesosphere near 90 km.Usually, at mid-latitudes, field-aligned irregularities cause non-specular trails, while in the polar region long-lasting irregularities are possibly sustained by charged meteor dust.The unusual meteor trails propagate downward and upward at speeds of 3.3-6.4 kms-1 along a slanted path length of 10.4 km between 87-93 km altitudes, merging in the middle and lasting for 8-10s. Here we propose that an electrical discharge is responsible for these trails. The corresponding horizontal electric field for the observed speeds is estimated up to 16.3 Vm-1 at 90 km.Both the long-lasting merging of two fast-moving plasma trails and the modest speed compared to those (~104 -105 ms -1 ) of lightning leader process and of jets (< 400 ms) occurring above thunderclouds likely suggest a new type of meteor-trail leader discharge occurring in the summer polar upper mesosphere
A dust-enshrouded tidal disruption event with a resolved radio jet in a galax...Sérgio Sacani
Tidal disruption events (TDEs) are transient flares produced when a star is ripped apart by the
gravitational field of a supermassive black hole (SMBH). We have observed a transient source in the
western nucleus of the merging galaxy pair Arp 299 that radiated >1.5 × 1052 erg in the infrared and radio
but was not luminous at optical or x-ray wavelengths. We interpret this as a TDE with much of its emission
reradiated at infrared wavelengths by dust. Efficient reprocessing by dense gas and dust may explain the
difference between theoretical predictions and observed luminosities of TDEs. The radio observations
resolve an expanding and decelerating jet, probing the jet formation and evolution around a SMBH.
Flaring from the_supermassive_black_hole_in_mrk335_studied_with_swift_and_nustarSérgio Sacani
Os comportamentos estranhos e desconcertantes dos buracos negros tornam-se cada dia menos misteriosos, com as novas observações feitas com as missões Swift e NuSTAR da NASA. Os dois telescópios espaciais registraram um buraco negro supermassivo no meio de uma gigantesca explosão de luz de raio-X, ajudando os astrônomos a tentarem resolver um grande quebra-cabeça: Como os buracos negros supermassivos emitem flares?
Os resultados sugerem que os buracos negros supermassivos emitem flares de raios-X, quando suas coroas circundantes, fontes de partículas extremamente energéticas, são atiradas ou lançadas para fora dos buracos negros.
“Essa é a primeira vez que nós somos capazes de linkar o lançamento da coroa com uma flare”, disse Dan Wilkins, da Universidade de Saint Mary em Halifax, no Canadá e principal autor do artigo que descreve os resultados na revista Monthly Notices of The Royal Astronomical Society. “Isso nos ajudará a entender como os buracos negros supermassivos alimentam alguns dos objetos mais brilhantes do universo”.
Os buracos negros supermassivos não emitem luz por si só, mas eles as vezes são circundados por discos de material quente e brilhante. A gravidade do buraco negro puxa o gás ao redor, aquecendo esse material e fazendo com que ele brilhe com diferentes tipos de luz. Outra fonte da radiação perto do buraco negro é a coroa. As coroas são feitas de partículas altamente energéticas que geram luz de raio-X, mas os detalhes sobre sua aparência, ou como elas se formam, ainda não são claros.
A Tectonic Origin for the Largest Marsquake Observed by InSightSérgio Sacani
The S1222a marsquake detected by InSight on 4 May 2022 was the largest of the mission, at 𝐴𝐴𝐴𝐴𝐴𝐴𝑀𝑀𝑤𝑤 4.7. Given its resemblance to two other large seismic events (S1000a and S1094b), which were associated with the formation of fresh craters, we undertook a search for a fresh crater associated with S1222a. Such a crater would be expected to be ∼300 m in diameter and have a blast zone on the order of 180 km across. Orbital images were targeted and searched as part of an international, multi-mission effort. Comprehensive analysis of the area using low- and medium-resolution images reveals no relevant transient atmospheric phenomena and no fresh blast zone. High-resolution coverage of the epicentral area from most spacecraft are more limited, but no fresh crater or other evidence of a new impact have been identified in those images either. We thus conclude that the S1222a event was highly likely of tectonic origin
Bright features have been recently discovered by Dawn on Ceres, which extend
previous photometric and Space Telescope observations. These features should produce
distortions of the line profiles of the reflected solar spectrum and therefore an apparent
radial velocity variation modulated by the rotation of the dwarf planet. Here we report
on two sequences of observations of Ceres performed in the nights of 31 July, 26-
27 August 2015 by means of the high-precision HARPS spectrograph at the 3.6-m
La Silla ESO telescope. The observations revealed a quite complex behaviour which
likely combines a radial velocity modulation due to the rotation with an amplitude of
⇡ ±6 m s
Introduction to AI for Nonprofits with Tapp NetworkTechSoup
Dive into the world of AI! Experts Jon Hill and Tareq Monaur will guide you through AI's role in enhancing nonprofit websites and basic marketing strategies, making it easy to understand and apply.
The x ray_outburst_of_the_galactic_centre_magnetar_sgr_j1745_2900_during_the_...Sérgio Sacani
Artigo descreve a pesquisa feita com a magnetar localizada próxima do buraco negro supermassivo da Via Láctea e que tenta explicar o comportamento estranho e incomum desse objeto misterioso.
C5.03: Ocean observations by the Global Change Observation Mission (GCOM) - K...Blue Planet Symposium
As a contribution to the climate variability monitoring, the Japan Aerospace Exploration Agency (JAXA) initiated the Global Change Observation Mission (GCOM). GCOM is a concept comprised of two polar-orbiting satellite series, spread over three generations to achieve long-term and consistent data records. The two satellite series are GCOM-W (Water) and GCOM-C (Climate). JAXA is implementing the first generation of the series. The GCOM-W satellite was launched on May 18, 2012 (Japan Standard Time) and started the continuous observation by the Advanced Microwave Scanning Radiometer-2 (AMSR2) from the A-Train orbit. The instrument has been showing stable performance and accumulating its data records. AMSR2 is capable of observing various oceanic and atmospheric geophysical parameters, including sea surface temperature (SST), sea surface wind speed, water vapor, cloud liquid water, precipitation, and sea ice. Particularly, nearly all-weather SST measurement by utilizing the characteristics of microwave observation is playing an important role in capturing dynamic changes of ocean phenomena, together with the time-proven infrared observations. The GCOM-C satellite is now under development and scheduled for launch in Japanese fiscal year 2016 to provide the continuous observations related to carbon cycle and radiation budget. The satellite will be equipped with the Second-generation Global Imager (SGLI) with some unique features including enhanced spatial resolution (250 m) for most of the visible channels, ultraviolet channels (380 nm), and polarization/multidirectional measurement capabilities. These features will provide the better understanding of the coastal phenomena through the detailed and accurate observations of coastal ocean colors and SST.
GW170817: Dawn of multi-messenger astronomy Amruta Jaodand
A bystander's view of how the detection of first neutron star merger seen by LIGO Scientific Collaboration and Virgo was followed up by electromagnetic observations. Timeline curated from discovery papers, twitter threads and GCN's
Evidence for Long-Lasting Electrical Leader Discharges in NonSpecular Meteor ...researchinventy
Unusual, non-specular, fast-movingmeteortrail echoes are observed in the summer polar upper mesosphere near 90 km.Usually, at mid-latitudes, field-aligned irregularities cause non-specular trails, while in the polar region long-lasting irregularities are possibly sustained by charged meteor dust.The unusual meteor trails propagate downward and upward at speeds of 3.3-6.4 kms-1 along a slanted path length of 10.4 km between 87-93 km altitudes, merging in the middle and lasting for 8-10s. Here we propose that an electrical discharge is responsible for these trails. The corresponding horizontal electric field for the observed speeds is estimated up to 16.3 Vm-1 at 90 km.Both the long-lasting merging of two fast-moving plasma trails and the modest speed compared to those (~104 -105 ms -1 ) of lightning leader process and of jets (< 400 ms) occurring above thunderclouds likely suggest a new type of meteor-trail leader discharge occurring in the summer polar upper mesosphere
A dust-enshrouded tidal disruption event with a resolved radio jet in a galax...Sérgio Sacani
Tidal disruption events (TDEs) are transient flares produced when a star is ripped apart by the
gravitational field of a supermassive black hole (SMBH). We have observed a transient source in the
western nucleus of the merging galaxy pair Arp 299 that radiated >1.5 × 1052 erg in the infrared and radio
but was not luminous at optical or x-ray wavelengths. We interpret this as a TDE with much of its emission
reradiated at infrared wavelengths by dust. Efficient reprocessing by dense gas and dust may explain the
difference between theoretical predictions and observed luminosities of TDEs. The radio observations
resolve an expanding and decelerating jet, probing the jet formation and evolution around a SMBH.
Flaring from the_supermassive_black_hole_in_mrk335_studied_with_swift_and_nustarSérgio Sacani
Os comportamentos estranhos e desconcertantes dos buracos negros tornam-se cada dia menos misteriosos, com as novas observações feitas com as missões Swift e NuSTAR da NASA. Os dois telescópios espaciais registraram um buraco negro supermassivo no meio de uma gigantesca explosão de luz de raio-X, ajudando os astrônomos a tentarem resolver um grande quebra-cabeça: Como os buracos negros supermassivos emitem flares?
Os resultados sugerem que os buracos negros supermassivos emitem flares de raios-X, quando suas coroas circundantes, fontes de partículas extremamente energéticas, são atiradas ou lançadas para fora dos buracos negros.
“Essa é a primeira vez que nós somos capazes de linkar o lançamento da coroa com uma flare”, disse Dan Wilkins, da Universidade de Saint Mary em Halifax, no Canadá e principal autor do artigo que descreve os resultados na revista Monthly Notices of The Royal Astronomical Society. “Isso nos ajudará a entender como os buracos negros supermassivos alimentam alguns dos objetos mais brilhantes do universo”.
Os buracos negros supermassivos não emitem luz por si só, mas eles as vezes são circundados por discos de material quente e brilhante. A gravidade do buraco negro puxa o gás ao redor, aquecendo esse material e fazendo com que ele brilhe com diferentes tipos de luz. Outra fonte da radiação perto do buraco negro é a coroa. As coroas são feitas de partículas altamente energéticas que geram luz de raio-X, mas os detalhes sobre sua aparência, ou como elas se formam, ainda não são claros.
A Tectonic Origin for the Largest Marsquake Observed by InSightSérgio Sacani
The S1222a marsquake detected by InSight on 4 May 2022 was the largest of the mission, at 𝐴𝐴𝐴𝐴𝐴𝐴𝑀𝑀𝑤𝑤 4.7. Given its resemblance to two other large seismic events (S1000a and S1094b), which were associated with the formation of fresh craters, we undertook a search for a fresh crater associated with S1222a. Such a crater would be expected to be ∼300 m in diameter and have a blast zone on the order of 180 km across. Orbital images were targeted and searched as part of an international, multi-mission effort. Comprehensive analysis of the area using low- and medium-resolution images reveals no relevant transient atmospheric phenomena and no fresh blast zone. High-resolution coverage of the epicentral area from most spacecraft are more limited, but no fresh crater or other evidence of a new impact have been identified in those images either. We thus conclude that the S1222a event was highly likely of tectonic origin
Bright features have been recently discovered by Dawn on Ceres, which extend
previous photometric and Space Telescope observations. These features should produce
distortions of the line profiles of the reflected solar spectrum and therefore an apparent
radial velocity variation modulated by the rotation of the dwarf planet. Here we report
on two sequences of observations of Ceres performed in the nights of 31 July, 26-
27 August 2015 by means of the high-precision HARPS spectrograph at the 3.6-m
La Silla ESO telescope. The observations revealed a quite complex behaviour which
likely combines a radial velocity modulation due to the rotation with an amplitude of
⇡ ±6 m s
Introduction to AI for Nonprofits with Tapp NetworkTechSoup
Dive into the world of AI! Experts Jon Hill and Tareq Monaur will guide you through AI's role in enhancing nonprofit websites and basic marketing strategies, making it easy to understand and apply.
Embracing GenAI - A Strategic ImperativePeter Windle
Artificial Intelligence (AI) technologies such as Generative AI, Image Generators and Large Language Models have had a dramatic impact on teaching, learning and assessment over the past 18 months. The most immediate threat AI posed was to Academic Integrity with Higher Education Institutes (HEIs) focusing their efforts on combating the use of GenAI in assessment. Guidelines were developed for staff and students, policies put in place too. Innovative educators have forged paths in the use of Generative AI for teaching, learning and assessments leading to pockets of transformation springing up across HEIs, often with little or no top-down guidance, support or direction.
This Gasta posits a strategic approach to integrating AI into HEIs to prepare staff, students and the curriculum for an evolving world and workplace. We will highlight the advantages of working with these technologies beyond the realm of teaching, learning and assessment by considering prompt engineering skills, industry impact, curriculum changes, and the need for staff upskilling. In contrast, not engaging strategically with Generative AI poses risks, including falling behind peers, missed opportunities and failing to ensure our graduates remain employable. The rapid evolution of AI technologies necessitates a proactive and strategic approach if we are to remain relevant.
Operation “Blue Star” is the only event in the history of Independent India where the state went into war with its own people. Even after about 40 years it is not clear if it was culmination of states anger over people of the region, a political game of power or start of dictatorial chapter in the democratic setup.
The people of Punjab felt alienated from main stream due to denial of their just demands during a long democratic struggle since independence. As it happen all over the word, it led to militant struggle with great loss of lives of military, police and civilian personnel. Killing of Indira Gandhi and massacre of innocent Sikhs in Delhi and other India cities was also associated with this movement.
A Strategic Approach: GenAI in EducationPeter Windle
Artificial Intelligence (AI) technologies such as Generative AI, Image Generators and Large Language Models have had a dramatic impact on teaching, learning and assessment over the past 18 months. The most immediate threat AI posed was to Academic Integrity with Higher Education Institutes (HEIs) focusing their efforts on combating the use of GenAI in assessment. Guidelines were developed for staff and students, policies put in place too. Innovative educators have forged paths in the use of Generative AI for teaching, learning and assessments leading to pockets of transformation springing up across HEIs, often with little or no top-down guidance, support or direction.
This Gasta posits a strategic approach to integrating AI into HEIs to prepare staff, students and the curriculum for an evolving world and workplace. We will highlight the advantages of working with these technologies beyond the realm of teaching, learning and assessment by considering prompt engineering skills, industry impact, curriculum changes, and the need for staff upskilling. In contrast, not engaging strategically with Generative AI poses risks, including falling behind peers, missed opportunities and failing to ensure our graduates remain employable. The rapid evolution of AI technologies necessitates a proactive and strategic approach if we are to remain relevant.
Unit 8 - Information and Communication Technology (Paper I).pdfThiyagu K
This slides describes the basic concepts of ICT, basics of Email, Emerging Technology and Digital Initiatives in Education. This presentations aligns with the UGC Paper I syllabus.
2024.06.01 Introducing a competency framework for languag learning materials ...Sandy Millin
http://sandymillin.wordpress.com/iateflwebinar2024
Published classroom materials form the basis of syllabuses, drive teacher professional development, and have a potentially huge influence on learners, teachers and education systems. All teachers also create their own materials, whether a few sentences on a blackboard, a highly-structured fully-realised online course, or anything in between. Despite this, the knowledge and skills needed to create effective language learning materials are rarely part of teacher training, and are mostly learnt by trial and error.
Knowledge and skills frameworks, generally called competency frameworks, for ELT teachers, trainers and managers have existed for a few years now. However, until I created one for my MA dissertation, there wasn’t one drawing together what we need to know and do to be able to effectively produce language learning materials.
This webinar will introduce you to my framework, highlighting the key competencies I identified from my research. It will also show how anybody involved in language teaching (any language, not just English!), teacher training, managing schools or developing language learning materials can benefit from using the framework.
Acetabularia Information For Class 9 .docxvaibhavrinwa19
Acetabularia acetabulum is a single-celled green alga that in its vegetative state is morphologically differentiated into a basal rhizoid and an axially elongated stalk, which bears whorls of branching hairs. The single diploid nucleus resides in the rhizoid.
Francesca Gottschalk - How can education support child empowerment.pptxEduSkills OECD
Francesca Gottschalk from the OECD’s Centre for Educational Research and Innovation presents at the Ask an Expert Webinar: How can education support child empowerment?
Model Attribute Check Company Auto PropertyCeline George
In Odoo, the multi-company feature allows you to manage multiple companies within a single Odoo database instance. Each company can have its own configurations while still sharing common resources such as products, customers, and suppliers.
1.4 modern child centered education - mahatma gandhi-2.pptx
Oct2013 Storm
1. The Coronal Mass Ejection of 29 Sep 2013
and Geomagnetic Storm of 2 Oct 2013
Peter T. Gallagher
School of Physics
Trinity College Dublin
2. Event Summary
• SDO observed a filament lift-off in the northwest quadrant of the Sun
(~W40) starting at ~2013-09-29T21:00Z.
• An asymmetric halo CME was observed in SOHO/LASCO images from22:24
UT. Apex velocity of ~897 km/s (LASCO) and 1097 km/s (STEREO B).
• ACE arrival time (L1): 2013-10-02T01:20Z
• GOES arrival time (1AU): 2013-10-02T02:00Z
• Geomagnetic storm start (Ireland): 2013-10-02T01:58Z
• Earth arrival times (models):
– NASA/GSFC SWRC Ensemble: 2013-10-02T04:1Z (+8/-12 hours)
– STOA:
2013-10-02T06:15Z (+/-10 hours)
8. Rough IDL Arrival Time Calculation
t_sdo = '2013-09-29T21:00Z’
au = 149e6
v_cme = 1096.
v_sw = 375.
v_ave = ( v_cme + v_sw ) / 2.
dt = au / v_ave
;
;
;
;
;
km
km/s
km/s
km/s
s
t_au = anytim( anytim( t_sdo ) + dt, /vms )
print, t_au
2-Oct-2013 05:14:05.656
This is ~4 hours later than observed arrival.
9. Conclusions
• STEREO –B CME velocity of 1097 km/s is less
than actual CME velocity as CME was directed
away from STEREO-B.
• STEREO-A CME velocities therefore likely to be
> STEREO-B velocities.
• From radial propagation model, need STEREOA CME velocity of 1200 km/s to get correct
arrival time at Earth (2-Oct-2013 ~01:00 UT).