Jove
Visualize
Contact Us
JoVE
x logofacebook logolinkedin logoyoutube logo
ABOUT JoVE
OverviewLeadershipBlogJoVE Help Center
AUTHORS
Publishing ProcessEditorial BoardScope & PoliciesPeer ReviewFAQSubmit
LIBRARIANS
TestimonialsSubscriptionsAccessResourcesLibrary Advisory BoardFAQ
RESEARCH
JoVE JournalMethods CollectionsJoVE Encyclopedia of ExperimentsArchive
EDUCATION
JoVE CoreJoVE BusinessJoVE Science EducationJoVE Lab ManualFaculty Resource CenterFaculty Site
Terms & Conditions of Use
Privacy Policy
Policies

Related Concept Videos

What is Climate?01:16

What is Climate?

21.2K
Climate refers to the prevailing weather conditions in a specific area over an extended period. As the saying goes, “Climate is what you expect. Weather is what you get.” Climate is influenced by geographic factors, such as latitude, terrain, and proximity to bodies of water.
21.2K
Tidal Forces01:06

Tidal Forces

3.5K
The origin of Earth's ocean tides has been a subject of continuous investigation for over 2000 years. However, the work of Newton is considered to be the beginning of the proper understanding of the phenomenon. Ocean tides are the result of gravitational tidal forces. These same tidal forces are present in any astronomical body; they are responsible for the internal heat that creates the volcanic activity on Io, one of Jupiter's moons, and the breakup of stars that get too close to...
3.5K
Radiation Pressure: Problem Solving01:09

Radiation Pressure: Problem Solving

929
The radiation pressure applied by an electromagnetic wave on a perfectly absorbing surface equals the energy density of the wave. The wave's momentum also gets transferred to the surface when an electromagnetic wave is entirely absorbed by it. The rate at which momentum is transmitted to an absorbing surface perpendicular to the propagation direction equals the force on the surface.
The average value of the rate of momentum transfer divided by the absorbing area represents the average force...
929
Radiation: Applications01:17

Radiation: Applications

1.9K
The average temperature of Earth is the subject of much current discussion. Earth is in radiative contact with both the Sun and dark space; it receives almost all its energy from the radiation of the Sun and reflects some of it into outer space. Dark space is very cold, about 3 K, so Earth radiates energy into it. For instance, heat transfer occurs from soil and grasses, the rate of which can be so rapid that frost can occur on clear summer evenings, even in warm latitudes.
The average...
1.9K
Kepler's First Law of Planetary Motion01:10

Kepler's First Law of Planetary Motion

5.9K
In the early 17th century, German astronomer and mathematician Johannes Kepler postulated three laws for the motion of planets in the solar system. He formulated his first two laws based on the observations of his forebears, Nikolaus Copernicus and Tycho Brahe.
Polish astronomer Nikolaus Copernicus put forth a theory that stated a heliocentric model for the solar system. According to this heliocentric theory, all the planets, including Earth, orbit the Sun in circular orbits.
On the other hand,...
5.9K
Reduced Mass Coordinates: Isolated Two-body Problem01:12

Reduced Mass Coordinates: Isolated Two-body Problem

2.5K
In classical mechanics, the two-body problem is one of the fundamental problems describing the motion of two interacting bodies under gravity or any other central force. When considering the motion of two bodies, one of the most important concepts is the reduced mass coordinates, a quantity that allows the two-body problem to be solved like a single-body problem. In these circumstances, it is assumed that a single body with reduced mass revolves around another body fixed in a position with an...
2.5K

You might also read

Related Articles

Articles linked to this work by shared authors, journal, and citation graph.

Sort by
Same author

Impact of limestone caves and seawater intrusion on coastal aquifer of middle Andaman.

Journal of contaminant hydrology·2023
Same author

Astrobiological Potential of Fe/Mg Smectites with Special Emphasis on Jezero Crater, Mars 2020 Landing Site.

Astrobiology·2022
Same author

Role of Satellite Sensors in Groundwater Exploration.

Sensors (Basel, Switzerland)·2016
Same author

Aqueous geochemistry of fluoride enriched groundwater in arid part of Western India.

Environmental science and pollution research international·2014
Same author

Identification of erosional and inundation hazard zones in Ken-Betwa river linking area, India, using remote sensing and GIS.

Environmental monitoring and assessment·2011
Same author

Sensible measures to guard India's groundwater supply.

Nature·2009

Related Experiment Video

Updated: Mar 11, 2026

Scattering And Absorption of Light in Planetary Regoliths
11:34

Scattering And Absorption of Light in Planetary Regoliths

Published on: July 1, 2019

11.1K

Cosmic Influence on the Sun-Earth Environment.

Saumitra Mukherjee1

  • 1Geology and Remote Sensing, School of Environmental Sciences, Jawaharlal Nehru University, New Delhi-110067, India. dr.saumitramukherjee@usa.net.

Sensors (Basel, Switzerland)
|November 23, 2016
PubMed
Summary

Geophysical changes precede shifts in the Sun-Earth environment, influenced by cosmic rays and solar activity. This connection may help predict earthquakes and extreme weather events.

Keywords:
SOHO satellite datachange in atmospherecosmicearthquakeextragalactic

More Related Videos

Surface Mapping of Earth-like Exoplanets using Single Point Light Curves
06:48

Surface Mapping of Earth-like Exoplanets using Single Point Light Curves

Published on: May 10, 2020

4.0K
Simulating Imaging of Large Scale Radio Arrays on the Lunar Surface
06:14

Simulating Imaging of Large Scale Radio Arrays on the Lunar Surface

Published on: July 30, 2020

5.4K

Related Experiment Videos

Last Updated: Mar 11, 2026

Scattering And Absorption of Light in Planetary Regoliths
11:34

Scattering And Absorption of Light in Planetary Regoliths

Published on: July 1, 2019

11.1K
Surface Mapping of Earth-like Exoplanets using Single Point Light Curves
06:48

Surface Mapping of Earth-like Exoplanets using Single Point Light Curves

Published on: May 10, 2020

4.0K
Simulating Imaging of Large Scale Radio Arrays on the Lunar Surface
06:14

Simulating Imaging of Large Scale Radio Arrays on the Lunar Surface

Published on: July 30, 2020

5.4K

Area of Science:

  • Geophysics
  • Space Physics
  • Astronomy

Background:

  • Solar cycles (periodic) and cosmic ray variations (episodic) influence the Sun-Earth environment.
  • The Sun's activity, monitored by the Solar and Heliospheric Observatory (SOHO) satellite, impacts Earth's geophysical systems.
  • Extragalactic influences on the Sun and Earth's environment exhibit both regular and unpredictable patterns.

Purpose of the Study:

  • To investigate the correlation between solar and cosmic anomalies and geophysical changes on Earth.
  • To explore the potential of the Star-Sun-Earth connection in predicting environmental events.

Main Methods:

  • Analysis of SOHO satellite data for geophysical changes.
  • Monitoring cosmic ray detectors for activity fluctuations.
  • Correlating solar and cosmic anomaly periods with Earth's environmental changes.

Main Results:

  • Geophysical changes were observed preceding sudden alterations in the Sun-Earth environment.
  • The Star-Sun-Earth connection demonstrates potential influence on Earth's thermosphere, atmosphere, ionosphere, and lithosphere.
  • Initial correlations suggest the possibility of predicting earthquakes and extreme weather patterns.

Conclusions:

  • The Sun-Earth environment is influenced by both periodic solar cycles and episodic cosmic events.
  • The Star-Sun-Earth connection offers a potential pathway for predicting significant geophysical and atmospheric events.
  • Further research into this connection could enhance our understanding of space weather impacts on Earth.