Environmental Bioscience & Human Transitional Behavior
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EME – this season update/ Autumn 2024
Listen Here: Scientists reveal the haunting sounds of Earth’s magnetic field flipping
A.abstract
So, why go to all this trouble to turn invisible magnetic fields into sound? “The intention, of course, is not to frighten people – it is a quirky way of reminding us that the magnetic field exists and although its rumble is a little unnerving, the existence of life on Earth is dependent on it,” Nielsen says, shedding light on the project’s purpose.
Indeed, Earth’s magnetic field is our invisible protector, a complex and dynamic bubble that shields us from cosmic radiation and the relentless solar wind. Generated by the swirling liquid iron in Earth’s outer core, this magnetic dynamo is essential for life as we know it.
October 10 2024 geomagnetic Storm
Abstract
In this short communication, we qualitatively analyze possible effects of the 10 October 2024 geomagnetic storm on accelerating the reentry of a Starlink satellite from low-Earth orbit (LEO). The storm took place near the maximum of solar cycle (SC) 25, which has shown to be more intense than SC24. Based on preliminary geomagnetic indices, the 10 October 2024, along with the 10 May 2024, were the most intense events since the well-known Halloween storms of October/November 2003. By looking at a preliminary version of the Dst index and two-line element (TLE) altitude data of the Starlink-1089 (SL1089) satellite, we observe a possible connection between storm main phase onset and a sharp decay of SL1089. The satellite was scheduled to reenter on 22 October, but it reentered on 12 October, 10 days before schedule. The sharp altitude decay of SL1089 revealed by TLE data coincides with the storm main phase onset. Therefore, we call for future research to establish the eventual causal relationship between storm occurrence and satellite orbital decay. As predicted by previous works, SC25 is already producing extreme geomagnetic storms with unprecedented satellite orbital drag effects and consequences for current megaconstellations in LEO.
Geomagnetic Storm effect and affect on Human Heart
Abstract
Introduction: Geomagnetic storms strongly affect the human cardiovascular system, misbalancing adaptive mechanisms and causing severe adaptive stress responses at all levels of body regulation. Most physiological changes occur after a defined period following geomagnetic climate alterations, this ‘delay period’ lasts for 2-3 days.
Methods and findings: In total, 4730 patients admitted between 2015 and 2017 due to Acute Coronary Syndrome (ACS) and acute onset of arrhythmias has been included into the study. Higher Time Varying Magnetic Field (TVMF) activity in low frequency ranges is associated with lower number of admissions due to ACS, while higher TVMF activity in high frequency ranges is associated with increased risk for ACS occurrence. The greater TVMF activity in low frequency ranges is associated with higher rates of admission due to cardiac arrhythmias. Additional ACS analysis showed that red blood cell count decreases with increased MF strength in low frequency ranges, while white blood cells and platelets count increases in the same MF frequency ranges. The highest serum osteocalcin level was found 3 days after certain MF strength changes in low frequency ranges in patients with ACS. Strong correlations were found between more than 2 cases of AMI per day and MF strength changes 2- and 3- days before admission.
Conclusion: Earth’s local magnetic field is strongly related to human cardiovascular system metabolism and neural regulation. Increased Magnetic field activity in low frequency ranges is associated with heart metabolism and may induce better cardiovascular health, while increased magnetic field activity in high frequency ranges leads to heart problems especially occurrence of ischemic heart disease and arterial hypertension.
Solar effect on Satellites
Magnetopause model
Geostationary satellites are usually protected to some extent from the effects of solar energetic particles by the Earth’s magnetic field. But, when the magnetopause, the abrupt boundary separating the solar wind from the Earth’s magnetic field, is pushed towards Earth (inside GEO orbits) by a major coronal mass ejection, some satellites will lose this protection and suffer damage from an increased flux of high energy particles.
Coronal holes appear as dark areas in the solar corona in extreme ultraviolet (EUV) and soft x-ray solar images. They appear dark because they are cooler, less dense regions than the surrounding plasma and are regions of open, unipolar magnetic fields. This open, magnetic field line structure allows the solar wind to escape more readily into space, resulting in streams of relatively fast solar wind and is often referred to as a high speed stream in the context of analysis of structures in interplanetary space.
Coronal holes can develop at any time and location on the Sun, but are more common and persistent during the years around solar minimum. The more persistent coronal holes can sometimes last through several solar rotations (27-day periods). Coronal holes are most prevalent and stable at the solar north and south poles; but these polar holes can grow and expand to lower solar latitudes. It is also possible for coronal holes to develop in isolation from the polar holes; or for an extension of a polar hole to split off and become an isolated structure. Persistent coronal holes are long-lasting sources for high speed solar wind streams. As the high speed stream interacts with the relatively slower ambient solar wind, a compression region forms, known as a co-rotating interaction region (CIR). From the perspective of a fixed observer in interplanetary space, the CIR will be seen to lead the coronal hole high speed stream (CH HSS).
Northern Hemisphere Autumn Equinox – September 21 2024 & ends on December 21 2024
Southern Hemisphere Spring Equinox – September 21 2024 & ends on December 21 2024
Last year on Earth – Human total Population have reach 8 billion:
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