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Return to Home will initiate and have the Halo Drone fly up to the altitude that you have set within the app settings, and take a straight line path from its current position to the Home Point indicated on your app.
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Make sure this altitude is set high enough to clear any trees or obstacles that may be in the path of the drone and your Home Point. Please note, that during this RTH procedure, you will still have control over your Halo Drone to help maneuver it around any obstacles.
You can abort the RTH procedure by pressing the P button on your remote to continue flying, however we do not recommend this. If the Halo Drone reaches critically low battery levels within another couple minutes , it will no longer initiate Return to Home, but will initiate an Emergency Auto-Land procedure and start landing directly over the location it currently is in to not risk having it stall out mid-flight and fall.
Do not cancel this landing procedure, the Halo Drone may not have enough power to operate properly and can lead to a crash. The current limit is determined by computational be generated in the simulation box. For example, limitations.
Three central blocks of particles were marked for highest mass resolution. Each block produces particles of the smallest mass. Adjacent blocks correspond to the four times lower resolution and produce 82 particles each.
The procedure is re- peated recursively until we reach the lowest level of resolution. The region of the highest resolution can have arbitrary shape. A large fraction of high resolution particles ends up in the central halo, which does not have any larger mass particles see insert in the bottom panel. At Fig. This was done to preserve halo was about 5 Mpc away. The halo had a fairly all small-scale perturbations present in the ini- typical merging history with M t track slightly tial spectrum of perturbations.
The local dynamical time for par- 0. The third halo was ticles moving in these regions is quite short. For 2 Mpc away from this pair.
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Moreover, the simulation was is only 0. There- in these regions will tend to grow. Even for small fore, the halo A can be considered as an example time steps errors exist and tend to alter the den- of a rather isolated well-relaxed halo. In many re- sity distribution in the centers of halos over some spects, this halo is similar to halos simulated by limited range of scales.
This gives about steps in more crowded environments. We have done a test run with twice are listed in Table 1. Some simula- achieved in the simulation.
Results ment, and, thus, they had fewer steps. Moore et al. Al- had no massive neighbors. The halo was located though the NFW and Moore et al.
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At the same time, if we rameters. Alterna- have a simple form and do not depend on the con- tively, if we choose to match the outer regions of centration.
The choice of the virial radius e. In this case, the dence on the concentration. In this case, one has formal concentration of the Moore et al.
In the case of tion is equal to CNFW. We show results for halos of low and high values of concentration representative of cluster- and low-mass galaxy ha- los, respectively. Each profile is normalized to have the typical dark matter dominated dwarf and LSB same virial mass and the same radius of the maximum galaxies.
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At the observationally interesting scales circular velocity. Top panels show the local logarithmic slope Note also that for galaxy-size e.
We can approximate the Moore et al. The mass resolution is thus tightly linked with the highest achievable spatial resolu- tion.
Columns present virial mass, radius, and the maximum cir- cular velocity of the halo. Here, as in the Fig. For vastly different mass and force parameters or the maximum circular velocities of resolutions the convergence is reached at these scales.
This is at odds with our convergence study in Kravtsov et al. In A1 , if considered including scales larger than two light of the results shown in Figure 4, it is clear formal resolutions, is consistent with conclusion that this is an artifact of underestimating true con- about the shallow central slope made in Kravtsov vergence scale and conclusions about shallow cen- et al.
Halo profiles the convergence scale. Figure 7 shows to the radius of 4 formal force resolutions. Check if the Camera is operating properly: Charge the camera, power it on separately, and turn AV Out mode off hold down arrow for 5 seconds until screen turns on again. The Halo Drone Flight battery is designed to warn users of any issues or conditions of the battery pack.
If LED 2 blinks slowly once per second , the battery has experienced an overcurrent discharge. If LED 2 blinks quickly 3 times per second , the battery has experienced an overcharge.
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Slowly discharge the battery. Stop charging and wait for the battery to cool.The mass resolution is thus tightly linked with the highest achievable spatial resolu- tion.
Even for small fore, the halo A can be considered as an example time steps errors exist and tend to alter the den- of a rather isolated well-relaxed halo. Halos B and parison project Frenk et al.
The ART code starts with paper in which we varied both mass and force reso- a uniform grid, which covers the whole computa- lution shows that for the ART simulations conver- tional box.
These comparisons and other tests initial conditions of the highest mass resolution. Figure 9 shows that all three profiles level.