• 0

Running Mac OS X on x86 PC!


Question

Recommended Posts

  • 0
Nearly running at 1GHZ.

;)

Can't get internet to work because it keeps bumping my wireless connection out when I bridge the two connections.

New build is very fast though.

Still a little slugish but its coming on really well.

What kind of processor do you have for PearPC to display such a high clockspeed? :blink:

  • 0

on my XP1800+ i get a 533Mhz G3 :p

anyone noticed how anything animating onscreen takes deteriorates the performance of the emu? like when starting an app, if you hide the dock, the app starts MUCH faster because there's no icon bouncing on the dock

  • 0

well i've managed to boot w/nic, but it isn't being recognize by OS X. The XP shows an active connection, and the DOS shows it is reciveing but not being filtered?

[iO/3c90x] indicate(00000010) mIntStatus now = 00000000

[iO/3c90x] acknowledge(00000010) mIntStatus now = 00000000

[iO/3c90x] EthTun: 250 bytes received. But they don't pass the filter.

[iO/3c90x] Not uploading, because: mUpStalled(=0) or UpListPtr == 0 (=00000000)

or not mRxPacketSize(=0)

Also the new build of pre.3 is slower than the one yesterday, so could someone send it to me?

  • 0
on my XP1800+ i get a 533Mhz G3 :p

anyone noticed how anything animating onscreen takes deteriorates the performance of the emu? like when starting an app, if you hide the dock, the app starts MUCH faster because there's no icon bouncing on the dock

You stole my idea! :angry: :angry:

:p

By the way, what are the keystrokes to get full-screen in the "other" build? I'm talking about the one that has right-click enabled. Shift-F12 doesn't work on that one.

Never mind. Got it. It's "F5".

Edited by eaglebtc
  • 0
sorry :blush: didn't mean to. i just posted because it's not just with the dock. anything that animates onscreen (even the friggin mouse) takes cpu power from the emu.

it's ok. :) I knew you didn't do it on purpose. Hence the :p below those harsh words.

  • 0

so i havent gotten the green light networking problem fixed

one think i have noticed is that

if u are running ure comp at 3-3.2 ghz pearpc shows around 900-950 mhz

If u r running 1.8 ghz like i am it will show 533 mhz

BUT remember with macs the speed is doubled to equal that of an intel processor

so if ure running 533 mhz on pearpc that is actually 1066mhz

  • 0

u sure i always heard that with the power pc processor that speed is doubled. Lets say u have an imac that is 200mhz that would be equal to a 400mhz pentium x processor. I really dont know if its true. But i read something about it in some Mac magazine

  • 0
u sure i always heard that with the power pc processor that speed is doubled. Lets say u have an imac that is 200mhz that would be equal to a 400mhz pentium x processor. I really dont know if its true. But i read something about it in some Mac magazine

ppc is generally faster, but usually not 2x as fast.

This topic is now closed to further replies.
  • Recently Browsing   0 members

    • No registered users viewing this page.
  • Posts

    • It's amazing that anyone still uses this bloated trash.
    • @Sayan...I have defended you at various points as I hope you know. This headline however is utter trash...shame on you sir!
    • An actual cosmic "Eye of Sauron" had been looking straight at us all along by Sayan Sen Image by Kovin P. Vasquez via Pexels | Not representative An international team of researchers has solved a long-standing mystery surrounding a distant blazar known as PKS 1424+240, helping explain why it produces some of the brightest high-energy gamma rays and cosmic neutrinos ever observed despite appearing to have a relatively slow-moving jet. The findings were published on June 6 in Astronomy & Astrophysics Letters. The study addresses a broader challenge in astrophysics: understanding how extreme cosmic objects accelerate particles to very high energies and produce very high-energy (VHE) photons and neutrinos. PKS 1424+240 is located billions of light-years from Earth. It has attracted attention for years because it is both a powerful source of VHE gamma rays and the brightest known neutrino-emitting blazar in the sky, according to observations by the IceCube Neutrino Observatory. It is also associated with one of the strongest peaks in IceCube's nine-year neutrino sky map A blazar is a type of active galactic nucleus powered by a supermassive black hole that pulls in surrounding matter and launches jets of plasma moving close to the speed of light. What makes blazars unique is their orientation. One of their jets points almost directly toward Earth, making them appear exceptionally bright across the electromagnetic spectrum and allowing scientists to study some of the most extreme physical processes in the Universe. The scientists exclaimed it's like the 'Eye of Sauron' in deep space. Usually, the brightest gamma-ray-emitting blazars are expected to have jets that appear to move very quickly. However, radio observations of PKS 1424+240 suggested that its jet was moving much more slowly, creating a contradiction that became part of a long-running problem known as the "Doppler factor crisis." To investigate, researchers analyzed 15 years of observations from the Very Long Baseline Array (VLBA), a network of 10 radio antennas spread across the continental United States, Hawaii and St. Croix. Using a technique called Very Long Baseline Interferometry (VLBI), astronomers combine signals from widely separated radio telescopes to create a virtual Earth-sized telescope capable of revealing extremely fine details. The team combined 42 polarization-sensitive radio images collected between 2009 and 2025, creating a much deeper and more detailed view of the jet than had previously been possible. The observations were carried out as part of MOJAVE (Monitoring Of Jets in Active galactic nuclei with VLBA Experiments), a long-running program that studies the brightness, polarization and magnetic field structures of jets produced by active galaxies. The project aims to better understand how activity near supermassive black holes is linked to high-energy radiation and neutrino emission. “When we reconstructed the image, it looked absolutely stunning,” said Yuri Kovalev, lead author of the study and Principal Investigator of the European Research Council-funded MuSES project at the Max Planck Institute for Radio Astronomy. “We have never seen anything quite like it — a near-perfect toroidal magnetic field with a jet, pointing straight at us.” The image revealed an unusual geometry. The researchers found that Earth lies almost directly in line with the jet, with a viewing angle of less than 0.6 degrees. In simple terms, astronomers are looking almost straight down the jet. This turned out to be the key to the mystery. Because the jet is aimed almost directly at Earth, a relativistic effect called Doppler boosting dramatically increases its apparent brightness. The study found that this effect boosts the emission by a factor of about 30 while also making the jet appear slower than it actually is. “This alignment causes a boost in brightness by a factor of 30 or more,” said Jack Livingston, a co-author at the Max Planck Institute for Radio Astronomy. “At the same time, the jet appears to move slowly due to projection effects — a classic optical illusion.” The nearly head-on view also gave scientists a rare look at the jet's magnetic field. Using polarized radio signals, they detected a clear toroidal, or doughnut-shaped, magnetic field component. The observations suggest the jet carries an electric current and that its magnetic field helps launch, shape and stabilize the flow of plasma. Researchers believe this magnetic structure may also play a key role in accelerating particles to energies high enough to produce both gamma rays and neutrinos. “Solving this puzzle confirms that active galactic nuclei with supermassive black holes are not only powerful accelerators of electrons, but also of protons — the origin of the observed high-energy neutrinos,” Kovalev said. The research was conducted under the MuSES (Multi-messenger Studies of Energetic Sources) project, which investigates how active galactic nuclei accelerate particles and generate different cosmic signals, including light and neutrinos. Scientists say understanding how protons are accelerated and linked to neutrino production remains one of the major unanswered questions in astrophysics. The findings help explain why some blazars can appear to have slow jets while still producing extremely bright high-energy emissions. More broadly, the study strengthens the link between relativistic jets, magnetic fields, gamma rays and high-energy neutrinos. Researchers say the results provide new clues about how some of the Universe's most powerful natural particle accelerators work and offer important insights for multimessenger astronomy, which combines different types of cosmic signals to study extreme events in space. Source: European Research Council, EDP Sciences This article was generated with some help from AI and reviewed by an editor. Under Section 107 of the Copyright Act 1976, this material is used for the purpose of news reporting. Fair use is a use permitted by copyright statute that might otherwise be infringing.
    • Gotenks98 is right... Outlook (new) is absolute trash. Doesn't Mozilla have an Enterprise Version of Firebird?
  • Recent Achievements

    • One Month Later
      lamborghiniv10 earned a badge
      One Month Later
    • Week One Done
      lamborghiniv10 earned a badge
      Week One Done
    • Reacting Well
      X-No-file earned a badge
      Reacting Well
    • One Month Later
      pestcontrol46 earned a badge
      One Month Later
    • Week One Done
      pestcontrol46 earned a badge
      Week One Done
  • Popular Contributors

    1. 1
      +primortal
      511
    2. 2
      PsYcHoKiLLa
      273
    3. 3
      Skyfrog
      75
    4. 4
      +Edouard
      72
    5. 5
      FloatingFatMan
      68
  • Tell a friend

    Love Neowin? Tell a friend!