nuclear chemistry

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neuclear reaction and types

A
Seminar on
Nuclear Chemistry
Submitted by
Vrushabh Tokse
BSc 3rd year 6th sem
Under the Guidance of
Chemistry Teachers
Department of Chemistry
Government Vidarbha Institute of Science & Humanities, Amravati,
(MS), India.

nuclear chemistry

nuclear chemistry

nuclear chemistry

nuclear chemistry

nuclear chemistry

nuclear chemistry

nuclear chemistry

nuclear chemistry

nuclear chemistry

nuclear chemistry

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The magnetic dynamo cycle of the Sun features a distinct pattern: a propagating region of sunspot emergence appears around 30° latitude and vanishes near the equator every 11 years (ref. 1). Moreover, longitudinal flows called torsional oscillations closely shadow sunspot migration, undoubtedly sharing a common cause2. Contrary to theories suggesting deep origins of these phenomena, helioseismology pinpoints low-latitude torsional oscillations to the outer 5–10% of the Sun, the near-surface shear layer3,4. Within this zone, inwardly increasing differential rotation coupled with a poloidal magnetic field strongly implicates the magneto-rotational instability5,6, prominent in accretion-disk theory and observed in laboratory experiments7. Together, these two facts prompt the general question: whether the solar dynamo is possibly a near-surface instability. Here we report strong affirmative evidence in stark contrast to traditional models8 focusing on the deeper tachocline. Simple analytic estimates show that the near-surface magneto-rotational instability better explains the spatiotemporal scales of the torsional oscillations and inferred subsurface magnetic field amplitudes9. State-of-the-art numerical simulations corroborate these estimates and reproduce hemispherical magnetic current helicity laws10. The dynamo resulting from a well-understood near-surface phenomenon improves prospects for accurate predictions of full magnetic cycles and space weather, affecting the electromagnetic infrastructure of Earth.

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The thermal continuum emission observed from accreting black holes across X-ray bands has the potential to be leveraged as a powerful probe of the mass and spin of the central black hole. The vast majority of existing ‘continuum fitting’ models neglect emission sourced at and within the innermost stable circular orbit (ISCO) of the black hole. Numerical simulations, however, find non-zero emission sourced from these regions. In this work, we extend existing techniques by including the emission sourced from within the plunging region, utilizing new analytical models that reproduce the properties of numerical accretion simulations. We show that in general the neglected intra-ISCO emission produces a hot-and-small quasi-blackbody component, but can also produce a weak power-law tail for more extreme parameter regions. A similar hot-and-small blackbody component has been added in by hand in an ad hoc manner to previous analyses of X-ray binary spectra. We show that the X-ray spectrum of MAXI J1820+070 in a soft-state outburst is extremely well described by a full Kerr black hole disc, while conventional models that neglect intra-ISCO emission are unable to reproduce the data. We believe this represents the first robust detection of intra-ISCO emission in the literature, and allows additional constraints to be placed on the MAXI J1820 + 070 black hole spin which must be low a• < 0.5 to allow a detectable intra-ISCO region. Emission from within the ISCO is the dominant emission component in the MAXI J1820 + 070 spectrum between 6 and 10 keV, highlighting the necessity of including this region. Our continuum fitting model is made publicly available.

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Getting into the tech field. what next

Google's Just Not That Into You: Understanding Core Updates & Search Intent

Google's Just Not That Into You: Understanding Core Updates & Search Intent

Google's Just Not That Into You: Understanding Core Updates & Search Intent

How to have difficult conversations

How to have difficult conversations

How to have difficult conversations

Introduction to Data Science

Introduction to Data Science

Introduction to Data Science

Time Management & Productivity - Best Practices

Time Management & Productivity - Best Practices

Time Management & Productivity - Best Practices

The six step guide to practical project management

The six step guide to practical project management

The six step guide to practical project management

Beginners Guide to TikTok for Search - Rachel Pearson - We are Tilt __ Bright...

Beginners Guide to TikTok for Search - Rachel Pearson - We are Tilt __ Bright...

Beginners Guide to TikTok for Search - Rachel Pearson - We are Tilt __ Bright...

Unlocking the Power of ChatGPT and AI in Testing - A Real-World Look, present...

Unlocking the Power of ChatGPT and AI in Testing - A Real-World Look, present...

Unlocking the Power of ChatGPT and AI in Testing - A Real-World Look, present...

12 Ways to Increase Your Influence at Work

12 Ways to Increase Your Influence at Work

12 Ways to Increase Your Influence at Work

nuclear chemistry

1. A Seminar on Nuclear Chemistry Submitted by Vrushabh Tokse BSc 3rd year 6th sem Under the Guidance of Chemistry Teachers Department of Chemistry Government Vidarbha Institute of Science & Humanities, Amravati, (MS), India.