Il Governo Netanyahu è una fabbrica di fake news, a Khan Younis è stato tutto distrutto e non cè più vita, mentre Rafah sta bruciando. La notte del 27 Maggio a Rafah si è assistito ad una notte orribile, con l’odore di polvere da sparo mescolato a corpi in fiamme, in un nuovo massacro che ha preso di mira le tende degli sfollati in aree che l’esercito israeliano dell’IDF ha ritenuto “aree umanitarie sicure” che di sicuro hanno avuto poco o niente.
Fonte: Il Fatto Quotidiano
English translate
DIARY FROM GAZA: THERE IS NO LIFE IN KHAN YOUNIS, THE STINK OF BURNED BODIES IN RAFAH
ISRAEL-HAMAS WAR EIGHTH MONTH NOVEMBER 2023-JUNE 2024
Netanyahu Government is a fake news factory, in Khan Younis everything has been destroyed and there is no life left, while Rafah is burning. The night of May 27th in Rafah witnessed a horrible night, with the smell of gunpowder mixed with burning bodies, in a new massacre that targeted the tents of displaced people in areas that the Israeli army IDF deemed “humanitarian safe areas” who certainly had little or nothing.
Diario da #Gaza: “A #KhanYounis non c’è vita, a #Rafah la puzza di corpi bruciati”. Diary from #Gaza: “In Khan Younis there is no life, in Rafah the stench of burnt bodies”.#IlFattoQuotidiano
6 Giugno 2024
— Alessio Brancaccio 🇵🇸 🍉🐺 (@bralex84) June 7, 2024
Dott. Alessio Brancaccio, tecnico ambientale Università degli Studi di L’Aquila, membro della Fondazione Michele Scarponi Onlus, ideologo e membro del movimento ambientalista Ultima Generazione A22 Network per contrastare il Riscaldamento Globale indotto artificialmente dalla Geoingegneria Solare SRM
A coronal mass ejection impact has been detected at the DSCOVR space craft. The solar wind speed hasn't increased much but the strength of the interplanetary field has significantly increased to about 20nT with a consistent southward component of about -17nT. Geomagnetic storm… pic.twitter.com/8NptueHUWf
A coronal mass ejection launched by an impulsive X1.6 solar flare that occurred yesterday is expected to arrive as a glancing blow late tomorrow, 5 May. The bulk of the coronal mass ejection is heading well north of our planet but a glancing blow should not be ruled out. Storm… pic.twitter.com/QcAadbPx5d
Major X-class solar flares equal major coronal mass ejections? Unfortunately that is not always the case. Today's X4.5 solar flare from sunspot region 3663 might have been the third strongest solar flare of the current Solar Cycle, it was yet another solar flare that was not or… pic.twitter.com/NtlGgQmaGx
Major X-class solar flares equal major coronal mass ejections? Unfortunately that is not always the case. Today's X4.5 solar flare from sunspot region 3663 might have been the third strongest solar flare of the current Solar Cycle, it was yet another solar flare that was not or… pic.twitter.com/NtlGgQmaGx
Two earth-directed asymmetrical coronal mass ejections were launched today due to the M and X-class activity from sunspot region 3664. Both are expected to arrive late on 10 May or early on 11 May. Moderate G2 geomagnetic storm conditions are possible after they arrive. More… pic.twitter.com/7hdyKSHpMN
Sunspot region 3664 remains very active and since our last update two more earth-directed coronal mass ejections were launched. One from an X1.0 flare and one from an X2.2 flare. The CMEs can be seen on the animations from SOHO/LASCO below.
The first of the anticipated coronal mass ejections has arrived at STEREO Ahead, a satellite slightly closer to the Sun than DSCOVR. The impact has been significant there with a maximum interplanetary magnetic field Bt value of 41nT and a minimum Bz value of -33nT at the time of… pic.twitter.com/AFw6X6p7jQ
For the first time since the Halloween Solar Storms of 2003 we have now officially reached the Extreme G5 geomagnetic storm threshold at 22:54 UTC.
With an observed Dst at -348 this is now one of the all-time strongest geomagnetic storms of the modern era only rivaled by the… pic.twitter.com/y8aHeFssOI
Midst among the excitement of the very first Extreme G5 geomagnetic storm since 2003, sunspot region 3664 continued doing what is is best at: producing major solar flares. It produced it's strongest solar flare thus far and the second strong solar flare of the current Solar… pic.twitter.com/G4ImkAr42j
Di recente abbiamo visto l’aurora boreale perfino in alcune zone dell’Italia. Questo insolito evento è stato innescato da una fortissima tempesta solare che ha influenzato il movimento del campo magnetico terrestre. Il Sole sta raggiungendo il punto massimo di attività in un ciclo di 11 anni. Ma cosa significa questo e cosa dobbiamo aspettarci? Non solo spettacolari aurore nel cielo, ma anche tempeste geomagnetiche che potrebbero danneggiare infrastrutture come le reti elettriche e i satelliti in orbita.
Il picco dell’attività solare
Posizione della macchia solare. Credit: NSF / NSO / AURA
È qui che entrano in gioco i potenziali problemi: un campo magnetico in movimento può generare corrente (Forza Elettro Motrice FEM) in qualsiasi cosa conduca elettricità(Legge di Faraday). Nelle infrastrutture moderne, la corrente si genera nelle linee elettriche, nei binari ferroviari e nelle condutture sotterranee. Anche la velocità di questo movimento è importante e viene monitorata misurando quanto il campo magnetico sia disturbato. Più a rischio sono le tubazioni metalliche che si corrodono quando la corrente elettrica le attraversa. Questo non è un effetto istantaneo, ma si verifica un lento accumulo di materiale erosivo. Ciò può avere un effetto molto forte sulle infrastrutture.
I problemi del Sole per i satelliti
I satelliti hanno una quantità limitata di messa a terra e una sovratensione elettrica può distruggere strumenti e comunicazioni. Quando un satellite perde le comunicazioni, viene definito satellite zombie e spesso viene perso completamente, causando una perdita molto elevata di investimenti. Non possiamo vedere questo cambiamento, ma la precisione del sistema di localizzazione in stile GPS può essere fortemente influenzata, poiché la lettura della posizione dipende dal tempo impiegato tra il dispositivo e un satellite. Gli stessi cambiamenti possono influenzare anche la velocità della larghezza di banda di Internet via satellite e le cinture di radiazioni del pianeta. Si tratta di particelle cariche altamente energetiche, per lo più elettroni, a circa 13.000 km dalla superficie terrestre.
The Sun is about to reach its maximum point of activity in an 11-year cycle. Here’s what it means.
Index hide
1 The peak of solar activity
2 The Sun’s problems for satellites
We recently saw the Northern Lights even in some areas of Italy. This unusual event was triggered by a very strong solar storm that affected the movement of the Earth’s magnetic field. The Sun is reaching its highest point of activity in an 11-year cycle. But what does this mean and what should we expect? Not only spectacular auroras in the sky, but also geomagnetic storms that could damage infrastructure such as electricity grids and orbiting satellites.
The peak of solar activity
Position of solar sunspot. Credit: NSF / NSO / AURA
This is where the potential problems come in: a moving magnetic field can generate current (Electro Driving Force EDF) in anything that conducts electricity (Faraday’s Law). In modern infrastructure, current is generated in power lines, railroad tracks, and underground pipelines. The speed of this movement is also important and is monitored by measuring how much the magnetic field is disturbed. Metal pipes that corrode when electric current passes through them are more at risk. This is not an instantaneous effect, but a slow accumulation of erosive material occurs. This can have a very strong effect on infrastructure.
The problems of the Sun for satellites
Satellites have a limited amount of grounding, and an electrical surge can destroy instruments and communications. When a satellite loses communications, it is called a zombie satellite and is often lost completely, causing a very large loss of investment. We can’t see this change, but the accuracy of the GPS-style tracking system can be greatly affected, as the location reading depends on the time taken between the device and a satellite. The same changes can also affect satellite Internet bandwidth speeds and the planet’s radiation belts. These are highly energetic charged particles, mostly electrons, about 13,000 km from the Earth’s surface.
Dott. Alessio Brancaccio, tecnico ambientale Università degli Studi di L’Aquila, membro della Fondazione Michele Scarponi Onlus, ideologo e membro del movimento ambientalista Ultima Generazione A22 Network per contrastare il Riscaldamento Globale indotto artificialmente dalla Geoingegneria Solare SRM
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