The Emergence of Extortion as a Growing Ransomware Threat

Cyber ​​criminals are Their efforts to maximize disruption and force payment of ransom demands have become more aggressive and new extortion tactics are now being implemented.

In early November, the notorious ALPHV ransomware gang, also known as BlackCat, used an unprecedented extortion tactic, weaponizing the U.S. government’s new data breach disclosure rules against one of the gang’s own victims. I tried. ALPHV has filed a complaint with the U.S. Securities and Exchange Commission (SEC), alleging that digital lending provider MeridianLink failed to disclose what the gang calls a “significant breach of customer data and operational information.” did. The gang took the credit..

“We would like to draw your attention to a concerning issue regarding MeridianLink’s compliance with the recently adopted Cybersecurity Incident Disclosure Regulations,” ALPHV wrote. “We are aware that MeridianLink has failed to file the required disclosures under Item 1.05 of Form 8-K within the required four business days, as required by new SEC rules.”

ALPHV’s latest extortion campaign is the first of what is expected to be a trend in the coming months after the rule goes into effect. Although novel, this is not the only aggressive tactic used by ransomware and extortion gangs.

Hackers, typically known for deploying ransomware, are increasingly resorting to “double extortion” tactics, where in addition to encrypting a victim’s data, they also threaten to release stolen files if a ransom demand is not paid. We are transitioning. Some people go further with “.”triple “Extortion” attack. As the name suggests, hackers use her three-pronged approach to extort money from victims by extending blackmail and ransom demands to the original victim’s customers, suppliers, and associates. To do. These tactics have been used by the hackers behind the widespread MOVEit mass hack, marking a significant milestone in the trend of extortion attempts that do not use encryption.

While vague definitions may not seem like the biggest cybersecurity issue facing organizations today, the distinction between ransomware and extortion is important. Especially since defenses against these two types of cyberattacks can be very different. This distinction also helps policy makers learn what ransomware trends are and whether anti-ransomware policies are working.

What is the difference between ransomware and extortion?

Ransomware Task Force I will explain Ransomware is “an evolving form of cybercrime in which criminals remotely infiltrate computer systems and either restore data or demand a ransom in exchange for not releasing the data.”

In reality, ransomware attacks can have far-reaching effects. In an analysis with TechCrunch, ransomware experts Allan Liska, a threat intelligence analyst at Recorded Future, and Brett Callow, a threat analyst at Emsisoft, explained that ransomware, broadly defined, is a collection of content on an insecure Elasticsearch instance. From a “$50 attack” to a devastating “encryption-based attack that poses a life threat to hospitals”.

“But obviously they’re very different animals,” Liska and Callow said. “One is an opportunistic porch pirate who steals Amazon deliveries, and the other is a team of thugs who break into homes, terrorize families, and take away all their possessions.”

Researchers say there are similarities between “encryption and extortion” attacks and “extortion-only attacks,” including their reliance on brokers selling access to compromised networks. But there are also important differences between the two, especially when it comes to victim clients, vendors, and customers, whose own sensitive data may be caught up in an extortion-only attack.

“We’ve seen this play out repeatedly, where attackers organize stolen data to find the largest or most well-known organizations and launch attacks against them. “This is not a new tactic,” Liska and Callow said, noting that one ransomware group claims to have hacked a major technology company, when in fact it hacked a little-known technology vendor. He gave an example of data theft.

“Preventing attackers from encrypting files on your network is one thing, but how do you protect the entire data supply chain?” Liska and Callow said. “In fact, many organizations don’t think about their data supply chain… yet each point in that supply chain is vulnerable to data theft and extortion attacks.”

We need a more precise definition of ransomware

Authorities have long prevented hacked organizations from paying ransom demands, but it’s not always an easy decision for companies victimized by hackers.

In encryption and extortion attacks, companies have the option of paying a ransom demand to obtain the key to decrypt their files. However, if you pay a hacker using aggressive extortion tactics to delete your stolen files, there is no guarantee that the hacker will actually delete them.

This was demonstrated in the recent ransomware attack on Caesars Entertainment, which rewarded hackers in an effort to prevent the release of stolen data. In its own admission, Caesars told regulators that it had “taken steps to ensure that the data stolen by the wrongdoers is deleted, but we cannot guarantee the outcome.”

“In fact, we should assume they won’t do that,” Liska and Callow said, referring to claims that the hackers would delete the data they stole.

“With a better definition of ransomware that accounts for the distinction between different types of attacks, organizations should be able to identify any type of ransomware, whether it occurs within their own network or a third-party network. We will be able to better plan and respond to Were attacks, Liska and Callow said.

Source: techcrunch.com

The Threat of Cool Star’s Strong Winds to Exoplanets

Artist’s illustration of a stellar planetary system. You can clearly see the stellar wind orbiting the star and its effect on the planet’s atmosphere.Credit: AIP/ K. Riebe/ J. Fohlmeister, editor

A groundbreaking study reveals that cold stars with strong magnetic fields generate powerful stellar winds, providing important information for assessing the habitability of exoplanetary systems.

A study led by scientists at the Potsdam Leibniz Institute for Astrophysics (AIP) uses cutting-edge numerical simulations to systematically characterize the properties of stellar winds in a sample of cold stars for the first time. Ta. They found that stars with stronger magnetic fields generate stronger winds. These winds create unfavorable conditions for the survival of planetary atmospheres, thus affecting the habitability of these systems.

Cool star classification

The Sun is one of the most abundant stars in the universe, known as “cool stars.” These stars are divided into four categories (F-type, G-type, K-type, and M-type) that differ in size, temperature, and brightness. The Sun is a fairly average star and belongs to category G. Stars that are brighter and larger than the Sun belong to category F, while K stars are slightly smaller and cooler than the Sun. The smallest and faintest star is the M star, also known as a “red dwarf” because of the color in which it emits most of its light.

Solar wind and its effects

Satellite observations have revealed that, apart from light, the sun continuously emits a stream of particles known as the solar wind. These winds travel through interplanetary space and interact with the planets of our solar system, including Earth. The beautiful displays of the Northern Lights near the North and South Poles are actually produced by this interaction. But these winds can also be harmful, as they can erode Earth’s stable atmosphere. Mars.

We know a lot about the solar wind, thanks in part to missions like Solar Orbiter, but the same isn’t true for other cool stars. The problem is that we can’t see these stellar winds directly, so we’re limited to studying their effects on the thin gas that fills the cavities between stars in galaxies. However, this approach has some limitations and can only be applied to a small number of stars. This has encouraged the use of computer simulations and models to predict various properties of stellar winds without the need for astronomer observations.

Pioneering research on the properties of stellar winds

In this regard, in collaboration with Cecilia Garaffo of the Harvard University Center for Astrophysics, doctoral student Judy Chevely of AIP’s Stellar Physics and Exoplanet Division, and scientist Julián D. Alvarado Gomez Dr. Katja Poppenhager, head of the department, assisted. The Smithsonian Institution conducted the first systematic study of the expected stellar wind properties for F, G, K, and M stars.

To this end, they performed numerical simulations using one of the most sophisticated models currently available, driven by the observed large-scale magnetic field distributions of 21 well-observed stars. I used it. The simulations were performed at the AIP and Leibniz-Rechenzentrum (LRZ) supercomputing facilities.

The research team investigated how star properties such as gravity, magnetic field strength, and rotation period affect the properties of the wind in terms of velocity and density. The results include a comprehensive characterization of stellar wind properties across spectral types and, in particular, challenge previous assumptions about stellar wind speeds when estimating associated mass loss rates from observations. This indicates that it needs to be reconsidered.

In addition, the simulations can predict the expected size of the Alfvén surface, the boundary between the stellar corona and the stellar wind. This information is the basis for determining whether planetary systems are affected by strong magnetic star-planet interactions. This interaction can occur when a planet’s orbit enters or is completely embedded in the Alfvén surface of its host star.

Impact on planetary systems

Their findings show that stars with magnetic fields larger than the Sun have faster winds. In some cases, stellar wind speeds can be up to five times faster than the average solar wind speed (typically 450 km/s). The study revealed how strong these stars’ winds are in their so-called “habitable zone,” defined as the orbital distance at which a rocky exoplanet can maintain liquid water on its surface and provide an Earth-like atmospheric pressure. It was evaluated as being strong. They found milder conditions around F- and G-type stars, comparable to those experienced by Earth around the G-type Sun, and increasingly harsh wind environments around K- and M-type stars. discovered. Such intense stellar winds have a strong impact on any atmosphere a planet might have.

Broader implications for exoplanet research

This phenomenon is well documented in heliophysics between rocky planets and the Sun, but not in exoplanetary systems. This requires estimates of stellar winds to assess processes similar to those seen between the solar wind and planetary atmospheres. This study is important from the perspective of habitability, as no information on stellar winds has been known for main-sequence stars F to M until now.

Although the study presented in this paper was performed on 21 stars, the results are general enough to apply to other cool main sequence stars. This study paves the way for future studies of stellar wind observations and their effects on planetary atmosphere erosion.

References: Judy J Chebly, Julián D Alvarado-Gómez, Katja Poppenhäger, and Cecilia Garraffo, “Quantifying the wind properties of cool main-sequence stars,” July 19, 2023. Royal Astronomical Society Monthly Notices.
DOI: 10.1093/mnras/stad2100

Source: scitechdaily.com