Q: (L) Okay. We've got quite a list of questions, so we might as well get on with it. Now, the first question is from Laurentien2, and he asks:
(Laurentien2) Are CMEs (Coronal Mass Ejections) related to the opening and closing of the Sun window?
(L) Well, that stopped me right there because, what is the Sun window? Now, I know the C’s have said that the center of spherical objects are windows, but I don't believe they ever said what they were windows to, and I don't think we ever asked that, did we? I mean...
(Laurentien2) Yeah, I thought, Laura, that they were a window to another realm, to another density. That's how I interpreted it.
(L) Right. So, I guess the first question we should ask before we even go any further with this, is, you said that the centers of spherical objects (and I think they even said all spherical objects, in a sense) were windows. So what is it a window to?
A: Depends on the object.
Q: (L) Okay. So, what is the window at the center of the Sun an opening to, or a window to?
A: Antiuniverse object.
Q: (L) Okay. So, the center of the Sun opens to an antiuniverse object. Is that antiuniverse object like an anti-Sun?
A: Close.
Q: (Ark) But you know, coming back to this question, once there is a window in a spherical object like the Sun, the window stays open as long as this spherical object remains a spherical object. And only what goes through this window can change or can fluctuate depending on activity.
A: Yes.
Q: (L) So, the window stays open because its function is as a window.
A: Yes.
Q: (L) Okay. So, there is no opening and closing of the Sun's window as long as the Sun continues to exist as a spherical object. And therefore, the question about coronal mass ejections is not relevant to the window state of the Sun. So, let's ask the next question: Are coronal mass ejections significant in some way, in a more than just, you know, ‘exploding thing’ sense?
A: Yes.
Q: (L) And what are they exactly?
A: Surges in heliogap field.
Q: (L) Okay. Surges in heliogap field. What… [laughs] I'm gonna do it, what is a heliogap field?
A: Field surrounding solar system.
Q: (L) Okay. So, I read about this Voyager spacecraft that they sent up years and years ago, and it was going into the outer reaches of the solar system and there were some strange effects on it when it started getting close to the reach of the Sun's... What would you call it? Its electrical reach.
(Andromeda) Electromagnetic field?
(L) Yeah, something like that. Yeah.
(Scottie) There's a name for it.
(Andromeda) Yeah, I know...
(L) I don't exactly remember what they call it. Do you know, honey?
(Joe) The heliofield.
(Niall) The heliosphere.
(L) That's it. Okay. So, does this have anything to do with the end of the heliosphere?
A: Yes.
Q: (L) And is there a gap outside this heliosphere?
A: Yes.
Q: (L) And you're saying that there was a surge. Where does that energy come from that surges across this gap and enters the heliosphere?
A: Other systems.
Q: (L) ‘Other systems’, as in solar systems or star systems?
A: Yes. Also galactic current.
Q: (L) So, there is a galactic current that's flowing in the galaxy, yes?
A: Yes.
Q: (L) And this galactic current crosses the gap into our heliosphere?
A: Yes.
Q: (L) And causes surges because it adds energy to our system. Is that it?
A: Yes.
Q: (L) And those surges can cause CMEs?
A: Yes.
Q: (L) And can those surges also cause very, very big ones?
A: Yes. Some surges can cause a star to explode.
Q: (L) Well, that's pleasant. Is that what's going to happen here?
A: No.
Q: (L) How do you know it's not going to happen? [Laughter]
A: Current is not that strong at present.
Q: (L) All right. Laurentien2, are you happy? Everything's okay now?
(Laurentien2) Yes, from what I understand, I'm happy, Laura. Sorry.
(L) Okay. I just wanted to make sure we handled your question with sufficient thoroughness. And we found out a few little things. [...]
